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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
Star in the constellation Hercules
of only 14.91 days. This system is the nearest example of a post-common-envelope binary. GJ 3991 B was first identified in 1997 by astronomers I. N.
GJ_3991
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
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
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 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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Planetary nebula located in the constellation Lyra
a common-envelope (CE) phase. The central star is a ∼140-kK white dwarf with a mass of ∼0.84 M☉. making it one of the hottest and most massive post-CE
ETHOS_1
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)
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
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
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
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
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
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
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
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
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
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
Hypothetical early-universe star with a black hole core
envelope of gas (which contains the bulk of the star's mass) held back by radiation pressure generated by the infalling gas. This overlying envelope is
Quasi-star
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Brief thermal runaway nuclear fusion in the core of low-mass stars
carbon–oxygen white dwarf. When hydrogen gas is accreted onto a white dwarf from a binary companion star, the hydrogen can fuse to form helium for a narrow range
Helium_flash
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
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
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
Hypothetical class of star that develops from a red dwarf
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Blue_dwarf_(red-dwarf_stage)
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
Collapsed core of a massive star
stars that have been detected are pulsars or a part of a binary system. Neutron stars in a binary system with a main sequence star can pull in large amounts
Neutron_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
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
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
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
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
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
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
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
Class of young variable stars
dissipate on timescales of up to 10 million years. Most T Tauri stars are in binary star systems. In various stages of their life, they are called young stellar
T_Tauri_star
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
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)
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
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
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
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
Main sequence star that is more luminous and bluer than expected
found among field stars, as a result of close binary interaction. Since the fraction of close binaries increases with decreasing metallicity, blue stragglers
Blue_straggler
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
Black hole formed by a collapsed star
a merger event of two smaller black holes. As of June 2020[update], the binary system 2MASS J05215658+4359220 was reported to host the smallest-mass black
Stellar_black_hole
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
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
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
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 types of stars
observations interpreted as originating in a black hole binary could really originate in a boson star binary. The invisible companion to a Sun-like star identified
Exotic_star
Star's outer shell from which light is radiated
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
Photosphere
Supernova at least ten times more luminous than a standard supernova
hydrogen envelope. Most hydrogen-poor events are classified as Type SLSN-I, with its visible radiation produced from a large expanding envelope of material
Superluminous_supernova
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
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
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
Type of star that is luminous, blue, and variable in brightness
Type IIb, or Type Ib supernovae, whereas binary stars undergo much-more-complex evolution through envelope stripping leading to less predictable outcomes
Luminous_blue_variable
Star not gravitationally bound to any galaxy
hypotheses have been suggested and published by astrophysicists. The most common hypothesis is that the collision of two or more galaxies can toss some stars
Intergalactic_star
Small patches of nebulosity associated with newly born stars
500 light-years) away from the Sun and is powered by a class I protostar binary. The bipolar jet is slamming into the surrounding medium at a velocity of
Herbig–Haro_object
Stellar classification distinguished by bright blue luminosity
Color–color diagram Strömgren sphere Kraft break Star systems Binary Contact Common envelope Eclipsing Symbiotic Multiple Cluster Open Globular Super Planetary
B-type_main-sequence_star
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
Type of star, larger and brighter than the Sun
energy-generation rate. The overall luminosity of the star decreases, its outer envelope contracts again, and the star moves from the red-giant branch to the horizontal
Giant_star
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
AzV 65 AzV 76 AzV 78 AzV 367 Barbá 2-2 BP Crucis (Wray 977 or GX 301-2), binary with a pulsar companion. Cygnus OB2-12 HD 5291 (Sk 56) HD 32034 (R62 in
Hypergiant
Stellar phenomenon
accuracy of 10K. For eclipsing binary stars – Eclipse mapping produces images and maps of spots on both stars. For giant binary stars – Very-long-baseline
Starspot
Supernova that ejects a large mass at unusually high velocity
to the speed of light. Binary systems are increasingly being studied as the best method for both stripping stellar envelopes to leave a bare carbon-oxygen
Hypernova
Outermost layer of a star's atmosphere
emission. However these stars do not have coronae, but the outer stellar envelopes emit this radiation during shocks due to thermal instabilities in rapidly
Stellar_corona
Stars that host planetary systems
are relatively common (as of October 2013 the spacecraft had found seven circumbinary planets out of roughly 1000 eclipsing binaries searched). One puzzling
Planet-hosting_star
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POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
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.
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’.
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.
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.
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.
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.
Male
Irish
Contracted form of Irish Gaelic Comhghán, COMGAN means "born together."
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).
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
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
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.
Male
Irish
Irish name COMYN means "shrewd."
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.
Male
Romanian
Romanian form of Greek Kosmos, COSMIN means "order, beauty."
Male
English
English masculine variant spelling of Scottish Cameron, CAMRON means "crooked nose."
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
Male
English
English form of Irish Colmán, COLMAN means "dove."
Boy/Male
Indian
Friend
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
 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
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
POST COMMON-ENVELOPE-BINARY
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