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Binary system consisting of a white dwarf and a main sequence star or a brown dwarf
A post-common-envelope binary (PCEB) or pre-cataclysmic variable is a binary system consisting of a white dwarf or hot subdwarf and a main-sequence star
Post-common-envelope_binary
Common gas atmosphere of a binary star system
astronomy, a common envelope (CE) is gas that contains a binary-star system. The gas does not rotate at the same rate as the embedded binary system. A system
Common_envelope
Stellar core remnant
Type Ia supernova, though this has been disputed. A post-common envelope binary (PCEB) is a binary consisting of a white dwarf or hot subdwarf and a closely
White_dwarf
Eclipsing post-common envelope binary star system in the constellation Serpens
NN Serpentis (abbreviated NN Ser) is an eclipsing post-common envelope binary system approximately 1670 light-years away. The system comprises an eclipsing
NN_Serpentis
Binary star system in the constellation Cygnus
J19383260+4603591 and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf B
Kepler-451
Supernova caused by a giant and compact star merging
the common envelope of a merging star. They may constitute 10–6 to 2 × 10–5 of all core collapse supernovae. In their model, iPTF14hls was a binary star
Common envelope jets supernova
Common_envelope_jets_supernova
Binary star system in the constellation Sculptor
have evaporated. WD 0137−349 represents the first confirmed post common envelope binary (PCEB) containing a white dwarf and a brown dwarf. As of 2018
WD_0137−349
Eclipsing binary star in the constellation Virgo
Draco QS Virginis – Eclipsing binary star in the constellation Virgo NN Serpentis – Eclipsing post-common envelope binary star system in the constellation
HW_Virginis
Planetary nebula in the constellation Pyxis
Kohoutek in 1961. The central star of the nebula—VW Pyxidis—is a post-common-envelope binary composed of a hot degenerate star and a cooler companion in a
K_1-2
Planet that orbits two stars instead of one
W. (2010-10-01). "Two planets orbiting the recently formed post-common envelope binary NN Serpentis". Astronomy and Astrophysics. 521: L60. arXiv:1010
Circumbinary_planet
Binary system in the constellation Serpens
planetary debris around white dwarfs Post common envelope binary WD 0137−349 another white dwarf-brown dwarf binary Farihi, J.; Parsons, S. G.; Gänsicke
SDSS_1557
Constellation in the northern celestial hemisphere
Lyra is Abell 46. The central star, V477 Lyrae, is an eclipsing post-common-envelope binary, consisting of a white dwarf primary and an oversized secondary
Lyra
Binary star in the constellation Virgo
with their hydrogen envelope completely stripped by a stellar companion. The companion is a red dwarf star. The eclipsing binary nature of NY Virginis
NY_Virginis
Constellation split into two non-contiguous parts
planet of at least 1.7 Jupiter-masses. NN Serpentis, an eclipsing post-common-envelope binary consisting of a white dwarf and a red dwarf, is very likely to
Serpens
Double star in the constellation Caelum
displays the same side to the heavier star. The system is also a post-common-envelope binary, and the red dwarf star is transferring material onto the white
RR_Caeli
Constellation in the southern celestial hemisphere
cannot be easily seen with amateur equipment. The system is a post-common-envelope binary and is losing angular momentum over time, which will eventually
Caelum
Star in the constellation Centaurus
HD 101584 is a suspected post-common envelope binary about 1,800 to 5,900 light-years distant in the constellation of Centaurus. The system is bright
HD_101584
Variable star in the constellation Taurus
type D2; and a K-type main sequence star (K2 V), together a post-common envelope binary. There are variations in the timing of the eclipses that were
V471_Tauri
System of two stars orbiting each other
Tohline, J. E.; J. E. Cazes; H. S. Cohl. "The Formation of Common-Envelope, Pre-Main-Sequence Binary Stars". Louisiana State University. Archived from the
Binary_star
Planetary nebula in the constellation Cygnus
planetary nebula, the stars must have formed a common envelope binary. Passing through a common envelope stage is often invoked as an explanation for the
Ou_5
Hermes, J. J. (2010). "Two planets orbiting the recently formed post-common envelope binary NN Serpentis". Astronomy and Astrophysics. 521: L60. arXiv:1010
List_of_exoplanet_firsts
J. (2010-10-01). "Two planets orbiting the recently formed post-common envelope binary NN Serpentis". Astronomy and Astrophysics. 521: L60. arXiv:1010
List of exoplanets and planetary debris around white dwarfs
List_of_exoplanets_and_planetary_debris_around_white_dwarfs
Stellar phenomenon
example, the orbital period variations in certain eclipsing post-common-envelope binaries are an order of magnitude larger than can be accommodated by
Applegate_mechanism
Type of barcode
CPC Binary Barcode is Canada Post's proprietary symbology used in its automated mail sortation operations. This barcode is used on regular-size pieces
CPC_Binary_Barcode
Substellar object
locked brown dwarfs orbiting around white dwarfs belong to the post common envelope binaries or PCEBs. Only eight confirmed PCEBs containing a white dwarf
Brown_dwarf
Highly magnetic type of cataclysmic variable binary star system
(2009-04-29). "Post common envelope binaries from the SDSS. VI. SDSS J120615.73+510047.0: a new low accretion rate magnetic binary". Astronomy and Astrophysics
Polar_(star)
Eclipsing binary star in the constellation Aquila
(2018). "The quest for stable circumbinary companions to post-common envelope SDB eclipsing binaries. Does the observational evidence support their existence
NSVS_14256825
Messaging protocol for web services
web services. It is an XML-based protocol consisting of three parts: an envelope, which defines the message structure and how to process it a set of encoding
SOAP
Process where a red giant star engulfs a planet
System including Mercury, Venus and possibly Earth. Common envelope Contact binary Interacting binary star Neutron star merger Stellar collision Leary,
Stellar_engulfment
Grouping of evolved cool luminous stars
undergoing fusion forming helium (known as hydrogen burning), and a very large envelope of material of composition similar to main-sequence stars (except in the
Asymptotic_giant_branch
Physical phenomenon of stars
star's mass. It can also occur when a star gradually loses material to a binary companion or due to strong stellar winds. Massive stars are particularly
Stellar_mass_loss
Italian and Australian astrophysicist
nebulae, binary stars that become large and close enough for their envelopes to interact, post common envelope binaries, and the role of binary interactions
Orsola_De_Marco
Blue star with strong helium lines
hundred million years. This may only happen if these two binary masses share the same type of envelope phase. It is believed this is the origin of the extreme
Helium_star
Variable star in the constellation Ursa Major
H.; et al. (June 1999), "Masses and Other Parameters of the Post-Common Envelope Binary BE Ursae Majoris", The Astrophysical Journal, 518 (2): 866–872
BE_Ursae_Majoris
Star in the constellation Centaurus
A 2014 publication hypothesized the star to be a contact binary, sharing a common envelope of material with a smaller yellow supergiant and secondary
HR_5171
Astrophysical phenomenon
Paczyński, B. (1976). "Common Envelope Binaries". In Eggleton, P.; Mitton, S.; Whelan, J. (eds.). Structure and Evolution of Close Binary Systems. IAU Symposium
Supernova
Internet protocol used for relaying e-mails
The protocol version in common use today has extensible structure with various extensions for authentication, encryption, binary data transfer, and internationalized
Simple_Mail_Transfer_Protocol
Hypothetical early-universe star with a black hole core
quasi-star, it is generally thought to consist of a photospheric star-like envelope (which contains the bulk of the star's mass) surrounded by a radiative
Quasi-star
Eclipsing binary star in the constellation Virgo
S.; et al. (2010). "Orbital Period Variations in Eclipsing Post Common Envelope Binaries". Monthly Notices of the Royal Astronomical Society. 407 (4):
QS_Virginis
von Harrach, S. (August 2022). "Eclipse timing variations in post-common envelope binaries: Are they a reliable indicator of circumbinary companions?"
List_of_exoplanet_extremes
Topics referred to by the same term
carrier and envelope of an electromagnetic wave Cerium, symbol Ce, a chemical element Cholesteryl ester Civil engineering Common envelope, gas containing
CE
Small number of stars that orbit each other
the Milky Way galaxy, with two-thirds of stars being single. Binary stars are the most common non-single stars. With multiple star systems, the number of
Star_system
Type of luminous supergiant star
A post-AGB star (pAGB, abbreviation of post-asymptotic giant branch) is a type of luminous low-mass supergiant star of intermediate mass in a very late
Post-AGB_star
Planetary nebula in the constellation Musca
velocity survey for post-common-envelope Wolf–Rayet central stars of planetary nebulae: first results and discovery of the close binary nucleus of NGC 5189★"
NGC_5189
Double stars that show a significant interaction between their components
complex and highly variable, and they are common sources of cataclysmic outbursts. A common type of interacting binary star is one in which one of the components
Interacting_binary_star
Nebula surrounding a dying star
the subsequent PN. At a point during or soon after the AGB envelope detachment, the envelope shape changes from roughly spherically symmetric to axially
Protoplanetary_nebula
Theoretical stellar remnant
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Black_dwarf
Star whose brightness fluctuates, as seen from Earth
1093/mnras/staa1455. Livio, Mario; Soker, Noam (June 1988). "The Common Envelope Phase in the Evolution of Binary Stars". Astrophysical Journal. 329: 764. Bibcode:1988ApJ
Variable_star
Hot, giant star of early spectral type
have helium burning cores, although they still have an extensive hydrogen envelope. They also have moderate masses around 0.5–1.0 M☉ so they are often much
Blue_giant
Flow of gas ejected from the upper atmosphere of a star
England: Cambridge University Press. ISBN 0521593980. OCLC 38738913. "Dust Envelopes". Stellar Physics. Astrophysical Institute Potsdam. Archived from the
Stellar_wind
Wang, Q.-S.; Voloshina, Irina (2018). "DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet". The Astrophysical
List of exoplanets discovered in 2018
List_of_exoplanets_discovered_in_2018
Stage of stellar evolution
in an overall reduction in luminosity, some contraction of the stellar envelope, and the surface reaching higher temperatures. Horizontal branch stars
Horizontal_branch
Hessman, F. V.; Deller, J. (2012). "The quest for companions to post-common envelope binaries. III. A reexamination of HW Virginis". Astronomy & Astrophysics
List of exoplanets discovered in 2012
List_of_exoplanets_discovered_in_2012
Part of a star
Circumstellar dust Common envelopes Stellar evolution Leao; Patrick De Laverny; Mekarnia; De Medeiros; Benoit Vandame (2007). "The circumstellar envelope of IRC+10216
Circumstellar_envelope
Type of large cool star
However, their outer envelope is lower in temperature, giving them a yellowish-orange hue. Despite the lower energy density of their envelope, red giants are
Red_giant
Type of neutron star with a strong magnetic field
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Magnetar
Hypothesized alternative to a black hole
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Gravastar
Two pulsars orbiting each other
A binary pulsar is a pulsar with a binary companion, often a white dwarf or neutron star. (In at least one case, the double pulsar PSR J0737-3039, the
Binary_pulsar
Star of luminosity class VI under the Yerkes spectral classification system
for their premature loss of their hydrogen envelope are unclear, but the interaction of stars in a binary star system is thought to be one of the main
Subdwarf
Early stage in the process of star formation
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Protostar
Changes to stars over their lifespans
giants or red supergiants if they are in binary systems close enough so that the companion star strips off the envelope as it expands, or if they rotate rapidly
Stellar_evolution
Class of astronomical objects
A symbiotic binary is a type of binary star system, often simply called a symbiotic star. They usually contain a white dwarf with a companion red giant
Symbiotic_binary
Hot, luminous star with a spectral type of A9 or earlier
supergiants from classes O9.5 to B2 are even more common than their main sequence counterparts. More post-main-sequence blue supergiants are observed than
Blue_supergiant
Isolated, small, and opaque nebula
Zinnecker, H. (10–15 April 2000). "Binary and multiple star formation in Bok globules". Birth and Evolution of Binary Stars, Poster Proceedings of IAU Symposium
Bok_globule
Constellations and Star Names to the Classical Period: An Annotated Bibliography (Un)Common Star Names This article includes an astronomy-related list of lists.
Lists of stars by constellation
Lists_of_stars_by_constellation
Planetary nebula in the constellation of Sagitta
photometry of the binary planetary nebula nuclei UU Sagitte and V477 Lyrae: oversized secondaries in post-common-envelope binaries", Monthly Notices of
Abell_63
Astronomical category of stars
astronomy, the term iron star has been used for two observed types of star: Binary stars with highly variable emission and stellar spectral type Fe a blue
Iron_star
Light from the stars
the H band, ascribing the CP to multiple scattering in circumstellar envelopes. Chrysostomou et al. found CP with q of up to 0.17 in the Orion OMC-1
Starlight
Central region of the Sun
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Solar_core
Coming together of two stars
by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms
Stellar_collision
Cosmic matter (remnant)
remaining in the expanding bubbles like T Pyxidis. Most novae require a close binary system, with a white dwarf and a main sequence, sub-giant, or red giant
Nova_remnant
Creation of chemical elements within stars
k_{r}} where kr is the reaction rate constant of each single elementary binary reaction composing the nuclear fusion process; k r = ⟨ σ ( v ) v ⟩ {\displaystyle
Stellar_nucleosynthesis
Stellar classification
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
K-type_main-sequence_star
Gravitational process studied in astronomy
the formation of a single star, must also account for the statistics of binary stars and the initial mass function. Most stars do not form in isolation
Star_formation
Type of star
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Strange_star
Grouping of stars by similar metallicity
small ultra metal-poor star, slightly smaller than the Sun, found in a binary system of the spiral arms in the Milky Way. The discovery opens up the possibility
Stellar_population
Pattern of stars recognized on Earth's night sky
right and also part of other asterisms. In many early civilizations, it was common to associate groups of stars in connect-the-dots stick-figure patterns.
Asterism_(astronomy)
Double star in the constellation Draco
"Characterizing the Cool KOIs. V. KOI-256: A Mutually Eclipsing Post-common Envelope Binary". The Astrophysical Journal. 767 (2). 111. arXiv:1304.1165. Bibcode:2013ApJ
KOI-256
Star whose atmosphere contains more carbon than oxygen
of carbon stars, belonging to the types C-J and C-H, are believed to be binary stars, where one star is observed to be a giant star (or occasionally a
Carbon_star
Class of astronomical objects that are X-ray sources
of a second to as much as several minutes. An X-ray pulsar is a type of binary star system consisting of a typical star (stellar companion) in orbit around
X-ray_pulsar
Low-mass supergiant that is almost devoid of hydrogen
core, causing the outer layers to expand rapidly. If the hydrogen in this envelope is consumed, the star becomes hydrogen-deficient and it contracts to form
Extreme_helium_star
Hypothetical star which gave life to the Sun
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Coatlicue_(star)
Compact exotic star which forms matter consisting mostly of quarks
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Quark_star
Set of non-stellar objects in orbit around a star
not engulfed move further out from the star. If an evolved star is in a binary or multiple system, then the mass it loses can transfer to another star
Planetary_system
Hypothetical hybrid star type
a binary system when one of the two stars goes supernova. Because no supernova is perfectly symmetric, and because the binding energy of the binary changes
Thorne–Żytkow_object
Heterogeneous class of stars with unusual spectra
Wolf–Rayet star is continually ejecting gas into space, producing an expanding envelope of nebulous gas. The force ejecting the gas at the high velocities observed
Wolf–Rayet_star
Binary pulsar–neutron star system in the constellation Vulpecula
millisecond pulsar and an X-ray binary. The aging companion star eventually engulfs the pulsar in a gaseous common envelope and their mutual orbit begins
PSR_J1946+2052
Type of neutron star with beams of radiation
useful tools for astronomers. For example, observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence of gravitational
Pulsar
Nuclear fusion reaction
small amount taken by the byproduct element, as added momentum. It is a common misconception that the above sequence ends at 28 56 N i {\displaystyle \
Alpha_process
Stellar explosion with a distinct red colour
co-existence of a bright flash with a cool post-flash object.[citation needed] In 2017 KIC 9832227, a binary star system, was predicted to merge and produce
Luminous_red_nova
Subdwarf star with spectral type O
pulsates with a frequency of 1.04 milliHertz. HD 49798 is a carbon poor X-ray binary at 830pc. US 708 is a hypervelocity star that exceeds the escape velocity
Subdwarf_O_star
Star in the stage when it has not yet reached the main sequence
acquiring mass from its surrounding envelope of interstellar dust and gas. After the protostar blows away this envelope, it is optically visible, and appears
Pre-main-sequence_star
Layer of a star's atmosphere
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Chromosphere
Stellar classification
pulses violently, with the star's gravity insufficient to hold its outer envelope. This results in significant mass loss and shedding. The ejected material
G-type_main-sequence_star
Star that has a supergiant luminosity class, with a spectral type of F or G
core-collapse supernova. The obvious candidate in such cases is always some form of binary interaction. Based on reports from Chinese astronomers in the 2nd/1st century
Yellow_supergiant
Hypothetical astronomical object
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Planck_star
Hypothetical gravitational object composed of matter
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Black star (semiclassical gravity)
Black_star_(semiclassical_gravity)
Planetary nebula in the constellation Monoceros
Boffin, Henri M. J.; Van Winckel, Hans (February 2019). "On the post-common-envelope central star of the planetary nebula NGC 2346". Monthly Notices of
NGC_2346
B-type star with forbidden emission lines
stars. Binary B[e] stars can produce discs of material as it is transferred from one star to another through roche lobe overflow. cPNB[e] are post-AGB stars
B(e)_star
Gas and dust surrounding a newly formed star
longer operates. It is believed that these disks consist of a turbulent envelope of plasma, also called the active zone, that encases an extensive region
Protoplanetary_disk
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
Female
English
 English name derived from the flower name which originally meant "a line of verse engraved on the inner surface of a ring," but later acquired the POSY means "bouquet, flower." Pet form of English Josephine, meaning "(God) shall add (another son)."Â
Male
English
English masculine variant spelling of Scottish Cameron, CAMRON means "crooked nose."
Surname or Lastname
English (most common in the West Country)
English (most common in the West Country) : nickname from Middle English swete ‘sweet’, ‘pleasant’, ‘agreeable’. The Old English bynames Swēt(a) (masculine) and Swēte (feminine) derived from this word survived into the early Middle English period, and may also be sources of the surname.Translation of German and Jewish (Ashkenazic) Suess.In New England, a translation of French Ledoux.
Girl/Female
American, Australian, British, Chinese, Christian, Danish, English, French, Gaelic, German, Greek, Indian, Irish, Italian, Portuguese
A Penelope; Wife of Odysseys; White Shoulder; Fionnula; Dream Weaver; Duck; Hard Working
Surname or Lastname
English
English : from a medieval personal name, a short form of Philpott.English : topographic name for someone who lived by a depression in the ground, from Middle English pot ‘drinking or storage vessel’ used in this transferred sense, or a habitational name from one of the minor places deriving their name from this word, in the sense ‘pit’, ‘hole’.English and North German (Lower Rhine-Westphalia) : metonymic occupational name for a potter, from Middle English, Middle Low German pot ‘pot’. See also Potter.North German : topographic name for someone living on a low-lying plot, from Low German dialect pÅt ‘puddle’.
Male
English
English form of Irish Colmán, COLMAN means "dove."
Boy/Male
Indian
Friend
Surname or Lastname
Swedish (common in Finland)
Swedish (common in Finland) : ornamental name formed with the common surname suffix -in and an unexplained first element.German : unexplained.English : unexplained.Spanish (FarÃn) : unexplained.
Surname or Lastname
English, Scottish, French, and Catalan
English, Scottish, French, and Catalan : topographic name for
someone who lived near a bridge, Middle English, Old French, Catalan
pont (Latin pons, genitive pontis).Catalan : habitational name from any of the numerous places named
with Pont.Dutch : variant of
Pond 2.A Pont from the Lorraine region of France is documented in Quebec City in
1640; Pont appears to be a secondary surname to
Male
Irish
Contracted form of Irish Gaelic Comhghán, COMGAN means "born together."
Surname or Lastname
English
English : occupational name for an innkeeper, from Middle English, Old French (h)oste ‘host’, ‘guest’.Danish (Høst) : nickname from høst ‘harvest’, ‘autumn’ (see Herbst).French : from Old French ost ‘army’, hence an occupational name for a soldier.Dutch : from the Germanic personal name Austa, meaning ‘east’.German : habitational name from either of two places called Host, near Koblenz and near Bitburg.
Male
Irish
Irish name COMYN means "shrewd."
Surname or Lastname
English (most common in East Anglia)
English (most common in East Anglia) : from Middle English reeve, an occupational name for a steward or bailiff, the precise character of whose duties varied from place to place and at different periods.
Female
English
Latin form of Greek Penelopeia, PENELOPE means "weaver of cunning." In mythology, this is the name of the patient wife of Odysseus who waited ten years for his return during which she refused several proposals of marriage by princes.
Surname or Lastname
English (but most common in Wales)
English (but most common in Wales) : from Lowis, Lodovicus, a Norman personal name composed of the Germanic elements hlod ‘fame’ + wīg ‘war’. This was the name of the founder of the Frankish dynasty, recorded in Latin chronicles as Ludovicus and Chlodovechus (the latter form becoming Old French Clovis, Clouis, Louis, the former developing into German Ludwig). The name was popular throughout France in the Middle Ages and was introduced to England by the Normans. In Wales it became inextricably confused with 2.Welsh : from an Anglicized form of the personal name Llywelyn (see Llewellyn).Irish and Scottish : reduced Anglicized form of Gaelic Mac Lughaidh ‘son of Lughaidh’. This is one of the most common Old Irish personal names. It is derived from Lugh ‘brightness’, which was the name of a Celtic god.Americanized form of any of various like-sounding Jewish surnames.This name was brought independently to New England by many bearers from the 17th century onward. William Lewis was one of the founders of Hartford, CT, (coming from Cambridge, MA, with Thomas Hooker) in 1635.
Surname or Lastname
English (now most common in northern Ireland)
English (now most common in northern Ireland) : probably a habitational name from a lost or unidentified place, most likely somewhere in Lancashire or Yorkshire.
Surname or Lastname
Scottish and northern Irish
Scottish and northern Irish : variant of Curzon.English (of Norman origin) : nickname from Old French corson, a diminutive of curt ‘short’ (see Court).
Male
English
 Anglicized form of Hebrew Rimmown, RIMMON means "pomegranate." In the bible, this is the name of several places, the name of a Benjamite of Beeroth.Â
Male
Romanian
Romanian form of Greek Kosmos, COSMIN means "order, beauty."
Surname or Lastname
English
English : from Middle English port ‘gateway’, ‘entrance’ (Old French porte, from Latin porta), hence a topographic name for someone who lived near the gates of a fortified town or city, typically, the man in charge of them. Compare Porter 1.English : topographic name for someone who lived near a harbor or in a market town, from the homonymous Middle English port (Old English port ‘harbor’, ‘market town’, from Latin portus ‘harbor’, ‘haven’, reinforced in Middle English by Old French port, from the same source).German : topographic name for someone who lived near a (city) gate, from Middle Low German porte (modern German Pforte) (see sense 1).Jewish (from Lithuania and Belarus) : unexplained.
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
Girl/Female
Hebrew
Lovely tune.
Boy/Male
Indian
Name of a king.
Female
English
Feminine variant spelling of English unisex Kelly, KELIA means "bright-headed."
Boy/Male
Tamil
The intelligent one, Name of Brihaspati, Planet jupiter, Spiritual preceptor, Epithet of Narayan
Boy/Male
Australian, French, Greek
Blessed
Boy/Male
Hindu, Indian, Tamil
Lord Murugan
Boy/Male
Australian, British, Christian, English, Scottish
Royal; Little Patrician; Little Noble
Boy/Male
Tamil
Kanhaiyalal | கநà¯à®¹à¯ˆà®¯à®¾à®²à®¾à®²
Lord Krishna
Male
English
Medieval English form of Roman Latin Maurice, MORRIS means "dark-skinned; Moor."
Girl/Female
Australian, Japanese
Child of Sato
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
n.
A post-temporal bone.
v. t.
To attach to a post, a wall, or other usual place of affixing public notices; to placard; as, to post a notice; to post playbills.
imp. & p. p.
of Envelop
n.
A piece of timber, metal, or other solid substance, fixed, or to be fixed, firmly in an upright position, especially when intended as a stay or support to something else; a pillar; as, a hitching post; a fence post; the posts of a house.
v. t.
To place in the care of the post; to mail; as, to post a letter.
n.
One of two suspending posts in a roof truss, or other framed truss of similar form. See King-post.
n. pl.
A club or association for boarding at a common table, as in a college, the members sharing the expenses equally; as, to board in commons.
v. i.
To board together; to eat at a table in common.
n.
See under 4th Post.
v. t.
To put a covering about; to wrap up or in; to inclose within a case, wrapper, integument or the like; to surround entirely; as, to envelop goods or a letter; the fog envelops a ship.
v. t.
Ruined or destroyed, either physically or morally; past help or hope; as, a ship lost at sea; a woman lost to virtue; a lost soul.
v.
Belonging to or shared by, affecting or serving, all the members of a class, considered together; general; public; as, properties common to all plants; the common schools; the Book of Common Prayer.
n.
Alt. of Envelop
v. i.
To have a joint right with others in common ground.
n.
That which envelops or surrounds; an envelop.
adv.
With post horses; hence, in haste; as, to travel post.
a.
Not common; unusual; infrequent; rare; hence, remarkable; strange; as, an uncommon season; an uncommon degree of cold or heat; uncommon courage.
n. pl.
A common; public pasture ground.
v. i.
To travel with post horses; figuratively, to travel in haste.
n.
A station, office, or position of service, trust, or emolument; as, the post of duty; the post of danger.