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Triple star system in the constellation Taurus
Lambda Tauri, Latinized from λ Tauri formally named Bibing, is a triple star system in the constellation Taurus. In 1848, the light from this system was
Lambda_Tauri
Binary star in the constellation Taurus
consisting of Theta² Tauri, Epsilon Tauri (named Ain), Delta³ Tauri, Delta¹ Tauri, Gamma Tauri, Alpha Tauri (Aldebaran), 71 Tauri and Lambda Tauri. Consequently
Theta_Tauri
Zodiac constellation straddling the celestial equator
Aurigae. Zeta Tauri (the proper name is Tianguan) is an eclipsing binary star that completes an orbit every 133 days. The star Lambda (λ) Tauri is an eclipsing
Taurus_(constellation)
Multiple star in the constellation Taurus
Gamma Tauri, Epsilon Tauri, Delta³ Tauri, Delta¹ Tauri, Alpha Tauri (Aldebaran), 71 Tauri and Lambda Tauri. Consequently, the Chinese name for γ Tauri itself
Gamma_Tauri
Binary star in the constellation Taurus
Tauri, Epsilon Tauri, Delta³ Tauri, Gamma Tauri, Alpha Tauri (Aldebaran), 71 Tauri and Lambda Tauri. Consequently, the Chinese name for Delta1 Tauri itself
Delta1_Tauri
Class of young variable stars
T Tauri stars (TTS) are a class of variable stars that are less than about ten million years old. This class is named after the prototype, T Tauri, a young
T_Tauri_star
Brightest sextuple star system 1.62 Lambda Scorpii Triple star system 1.64 1.59 Bellatrix Star 1.64 Gacrux Star 1.65 Beta Tauri Star 1.69 1.64 Alnilam Star 1
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Dark nebula in the constellation Orion
brown dwarfs and multiple T Tauri stars. The young population includes HK Orionis, a Herbig Ae/Be star and HI Orionis, a T Tauri star. The stellar population
Barnard_30
Measure of the strength of a spectral line
{\displaystyle W_{\lambda }=\int {F_{c}-F_{s} \over F_{c}}d\lambda =\int (1-F_{s}/F_{c})d\lambda .} Here, F c ( λ ) {\displaystyle F_{c}(\lambda )} represents
Equivalent_width
1145+017 b). Kappa Scorpii (Girtab) 480 ± 10 Scorpius B1.5 III 2.41 - 2.42 Lambda Tauri A 480 ± 10 Taurus B3 V +3.37 B A4 IV BL Crucis 480 ± 10 Crux M4-5III
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
Star in its early stage of evolution
={\frac {d\log(\lambda F_{\lambda })}{d\log(\lambda )}}} . Here λ {\displaystyle \lambda \,} is wavelength, and F λ {\displaystyle F_{\lambda }} is flux density
Young_stellar_object
Observatory in Urbana, Illinois, U.S.
series of papers in the Astrophysical Journal on eclipsing binaries Lambda Tauri, Algol, 1H Cassiopeiae (HR 8926), ellipsoidal variables π5 Orionis, and
Astronomical Observatory (University of Illinois Urbana-Champaign)
Astronomical_Observatory_(University_of_Illinois_Urbana-Champaign)
Stellar stream spanning from Eridanus to Pisces
has a mass of 770 M☉. The stream includes at least 6 naked eye stars: Lambda Tauri at 3.5 magnitude, 148 parsec distance; Omicron Aquarii at 4.7 magnitude
Pisces–Eridanus stellar stream
Pisces–Eridanus_stellar_stream
Gas and dust surrounding a newly formed star
circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may not be considered
Protoplanetary_disk
Peculiar star with unusually low amount of iron
A Lambda Boötis star is a type of chemically peculiar star which has an unusually low abundance of iron peak elements in its surface layers. One possible
Lambda_Boötis_star
Pattern of stars recognized on Earth's night sky
stars Gamma, Delta1, Delta2, Delta3, Epsilon, Theta Tauri, as well as the bright star Alpha Tauri (Aldebaran) which forms the red eye of the Bull. Other
Asterism_(astronomy)
Open star cluster in the constellation Orion
cluster is young and contains a large number of low-mass stars, some T Tauri stars and brown dwarfs. One notable member is LOri167, which is a wide binary
Lambda_Orionis_Cluster
Star in the constellation Orion
GW Orionis is a T Tauri type pre-main sequence hierarchical triple star system. It is associated with the Lambda Orionis star-forming region and has an
GW_Orionis
Constellation in the Southern Sky
molecular clouds (the Chamaeleon dark clouds) that are forming low-mass T Tauri stars. The cloud complex lies some 400 to 600 light years from Earth, and
Chamaeleon
Light from the stars
invoked by Bastien, Robert and Nadeau, to explain the CP measured in 6 T-Tauri stars at a wavelength of 768 nm. They found a maximum CP of q ∼ 7 × 10 −
Starlight
British writer, critic, and poet (born 1949)
transgender identity and transphobia ... hilarious and chilling". It won the 2016 Lambda Literary Award for Transgender Fiction. From 1982-1984 Kaveney was an editor
Roz_Kaveney
Event when planets are seen to pass one another
1825 09:10 Venus Delta-1 Tauri 44.4° West 11 July 1837 12:50 Mercury Eta Geminorum 17.8° West 9 May 1841 19:35 Venus 17 Tauri 9.2° East 27 September 1843
Planetary transits and occultations
Planetary_transits_and_occultations
Young stars of spectral types A and B
than F0 (in order to exclude T Tauri stars), Balmer emission lines in the stellar spectrum (in order to be similar to T Tauri stars), Projected location within
Herbig_Ae/Be_star
Small patches of nebulosity associated with newly born stars
of object. T Tauri was found to be a very young and variable star, and is the prototype of the class of similar objects known as T Tauri stars which have
Herbig–Haro_object
Constellation straddling the celestial equator
Orion as a hunter; an arrow he has shot is represented by Aldebaran (Alpha Tauri), with the same figure as other Western depictions. In Greek mythology,
Orion_(constellation)
Flow of gas ejected from the upper atmosphere of a star
pressure on dust condensing in the upper atmosphere of the stars. Young T Tauri stars often have very powerful stellar winds.[citation needed] Massive stars
Stellar_wind
Theoretical stellar remnant
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Black_dwarf
Early stage in the process of star formation
globule Dark nebula Young stellar object Protostar Pre-main-sequence star T Tauri star Herbig Ae/Be star Herbig–Haro object Theoretical concepts Accretion
Protostar
Peripheral nebular regions of the Orion Molecular Cloud Complex
eastern side, indicating active star formation. At least three of these are T Tauri stars, coinciding with IRAS or X-ray sources. NGC 1788 is a small reflection
Peripheral nebular regions of the Orion Complex
Peripheral_nebular_regions_of_the_Orion_Complex
Methods for estimating the age of a star
advanced evolutionary stages. When a roughly solar-mass star exhibits T Tauri variability, astronomers can locate the age of the star as being before
Stellar_age_estimation
Type of variable star
codes were used "nebular" or "rapidly irregular" variable stars such as T Tauri and Orion variables. The remaining irregular stars, cool slowly varying
Slow_irregular_variable
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Lists of stars by constellation
Lists_of_stars_by_constellation
Type of luminous supergiant star
eye, the brightest of which is 89 Herculis. Other examples include: RV Tauri R Scuti U Monocerotis Habing, Harm (1997). Paresce, Francesco (ed.). AGB
Post-AGB_star
α Crucis 0320 B0.5 IV, B1 V Southern 14 0.86 (0.75–0.95var) Aldebaran α Tauri 0065 K5 III Northern 15 0.96 (0.6–1.6var) Antares α Scorpii 0550 M1.5 Iab-Ib
List_of_brightest_stars
Small number of stars that orbit each other
the first quadruple star system with an Earth-sized planet. Xi Tauri (ξ Tau, ξ Tauri), located about 222 light years away, is a spectroscopic and eclipsing
Star_system
Star whose brightness fluctuates, as seen from Earth
Nebula. A well-known subtype of Orion variables are the T Tauri variables. Variability of T Tauri stars is due to spots on the stellar surface and gas-dust
Variable_star
Alpha Draconis, "Thuban" Ain ʽAyn the Eye (of the bull) عين عَيْن Epsilon Tauri Aladfar al-ʼUẓfūr the Talons (of the Swooping Eagle) الأظفر أُظْفُور Eta
List_of_Arabic_star_names
Hypothesized alternative to a black hole
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Gravastar
Constellation in the southern celestial hemisphere
216...44D. Mamajek, E. E.; Meyer, M. R.; Liebert, James (2002). "Post-T Tauri Stars in the Nearest OB Association". Astronomical Journal. 124 (3): 1670–1694
Crux
Region of an astronomical diagram
branch; and the Cepheid variables where it crosses the supergiants. RV Tauri variables are also often considered to lie on the instability strip, occupying
Instability_strip
Star that has a supergiant luminosity class, with a spectral type of F or G
low masses, including W Virginis variables, BL Herculis variables and RV Tauri variables. The Classical Cepheids are more luminous than the type II Cepheids
Yellow_supergiant
Type of star that is massive and luminous
receive spectral types with supergiant luminosity classes. For example, RV Tauri has an Ia (bright supergiant) luminosity class despite being less massive
Supergiant
Hypothetical astronomical object
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Planck_star
Type of star, larger and brighter than the Sun
blue giants. Examples: Meissa (λ Orionis A), an O-type giant. Alcyone (η Tauri), a B-type giant, the brightest star in the Pleiades; Thuban (α Draconis)
Giant_star
Hypothetical early-universe star with a black hole core
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Quasi-star
Stars with a supergiant luminosity class with a spectral type of K or M
Antares A Betelgeuse Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically thought to be a red supergiant
Red_supergiant
Constellation in the northern celestial hemisphere
harvest, was a constellation formed by Alpha Aurigae, Beta Aurigae, Beta Tauri, Theta Aurigae, and Iota Aurigae. Sanzhu or Zhu was one of three constellations
Auriga
Grouping of stars by similar metallicity
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar_population
Type of variable star
(Classical cepheids, Delta Scuti) Type II (BL Herculis, W Virginis, RV Tauri) RR Lyrae Rapidly oscillating Ap SX Phoenicis Blue-white with early spectra
Rapidly_oscillating_Ap_star
Isolated, small, and opaque nebula
globule Dark nebula Young stellar object Protostar Pre-main-sequence star T Tauri star Herbig Ae/Be star Herbig–Haro object Theoretical concepts Accretion
Bok_globule
Astronomical category of stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Iron_star
Type of neutron star with beams of radiation
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Pulsar
Curve on the Hertzsprung-Russell diagram representing stars of a particular age
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar_isochrone
originally Arabic: الذيل aḏ-ḏayl (the train, lit. 'the tail'). /əˈdɪl/ Ain ε Tauri Taurus Arabic The name is originally from Arabic: عين ʿayn ('eye') and was
List_of_proper_names_of_stars
Star formation process
0.4 pc ⋅ c s 0.2 km/s ⋅ ( n 10 3 cm − 3 ) − 1 / 2 . {\displaystyle \lambda _{\text{J}}={\frac {c_{\text{s}}}{(G\rho )^{1/2}}}\approx 0.4{\text{ pc}}\cdot
Jeans_instability
Large self-illuminated object in space
Tauri stars follow the Hayashi track—they contract and decrease in luminosity while remaining at roughly the same temperature. Less massive T Tauri stars
Star
Luminosity–temperature relationship in stars
After a protostar ends its phase of rapid contraction and becomes a T Tauri star, it is extremely luminous. The star continues to contract, but much
Hayashi_track
Hypothetical types of stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Exotic_star
Star in the stage when it has not yet reached the main sequence
is the pre-main sequence stage. An observed PMS object can either be a T Tauri star, if it has fewer than 2 solar masses (M☉), or else a Herbig Ae/Be star
Pre-main-sequence_star
Stellar classification
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
G-type_main-sequence_star
Magnetic field generated inside a star
gradually approach, but never quite reach, the state of zero rotation. A T Tauri star is a type of pre-main-sequence star that is being heated through gravitational
Stellar_magnetic_field
Supernova that ejects a large mass at unusually high velocity
0969. Bibcode:2008ApJ...680.1350F. doi:10.1086/529416. S2CID 118559576. Tauris, T. M.; Langer, N.; Moriya, T. J.; Podsiadlowski, Ph.; Yoon, S.-C.; Blinnikov
Hypernova
Coming together of two stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar_collision
Type of star
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Strange_star
Hypothetical class of star that develops from a red dwarf
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Blue_dwarf_(red-dwarf_stage)
Scatter plot of stars showing the relationship of luminosity to stellar classification
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Hertzsprung–Russell_diagram
Process of energy release of a contracting star or planet
globule Dark nebula Young stellar object Protostar Pre-main-sequence star T Tauri star Herbig Ae/Be star Herbig–Haro object Theoretical concepts Accretion
Kelvin–Helmholtz_mechanism
Constellation in the northern celestial hemisphere
mystery: first cataloged as an eclipsing binary, it was theorized to be an RV Tauri variable in 2002, but if so, it would be by far the hottest such variable
Lyra
Type of large cool star
K1.5 red-giant branch star Arcturus is 36 light-years away. Aldebaran (α Tauri) Arcturus (α Bootis) μ Leonis Gacrux (γ Crucis) Pollux (β Geminorum) Capella
Red_giant
Outermost layer of a star's atmosphere
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar_corona
Layer of a star's atmosphere
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Chromosphere
Creation of chemical elements within stars
section is proportional to π λ 2 {\textstyle \pi \,\lambda ^{2}} , where λ = h / p {\textstyle \lambda =h/p} is the de Broglie wavelength. Thus semi-classically
Stellar_nucleosynthesis
Stellar core remnant
Bibcode:2021NatAs...5.1170C. doi:10.1038/s41550-021-01445-6. Istrate, A.G.; Tauris, T.M.; Langer, N.; Antoniadis, J. (2014). "The timescale of low-mass proto-helium
White_dwarf
Dim, low mass stars on the main sequence
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Red_dwarf
Brief thermal runaway nuclear fusion in the core of low-mass stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Helium_flash
Astronomical objects of planetary size that did not form in orbit around a star
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Sub-brown_dwarf
Star of luminosity class VI under the Yerkes spectral classification system
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Subdwarf
Bookkeeping survey of stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Star_count
Micronesian navigator (1932–2010)
Arietis Murn Vega Vega Marigaht Seven Sisters Pleiades Uul Aldebaran Alpha Tauri Paiifung Tarazed Gamma Aquilae Mailap Altair Alpha Aquilae Paiyur Alshain
Mau_Piailug
Type of star with a prominent spectral line due to absorption from ionized mercury
Alpheratz α Andromedae B8IVmnp 2.06 Gienah Corvi γ Corvi A B8III 2.59 Maia 20 Tauri B8III 3.87 χ Lupi B9IV 3.96 Muliphein γ Canis Majoris B8II 4.10 φ Herculis
Mercury–manganese_star
Type of neutron star with a strong magnetic field
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Magnetar
Astronomical phenomenon
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Gravity_darkening
Changes to stars over their lifespans
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar_evolution
Astronomical object without the mass to sustain hydrogen fusion
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Substellar_object
Classification in astronomy
Bibcode:2020ApJ...895L..37B. doi:10.3847/2041-8213/ab672e. S2CID 218900539. Tauris, T. M.; J. van den Heuvel, E. P. (20 Mar 2003). Formation and Evolution
Compact_object
Hot, giant star of early spectral type
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Blue_giant
Star not gravitationally bound to any galaxy
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Intergalactic_star
Value in astrophysics
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Hayashi_limit
Astrophysical phenomenon
Bibcode:2013Natur.502..346N. doi:10.1038/nature12569. PMID 24132291. S2CID 4472977. Tauris, T. M.; Langer, N.; Moriya, T. J.; Podsiadlowski, P.; Yoon, S.-C.; Blinnikov
Supernova
Star of relatively small size and low luminosity
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Dwarf_star
Light emitted by the Sun
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Sunlight
Star's outer shell from which light is radiated
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Photosphere
Type of interstellar cloud
matching molecular clouds’ internal timescales. Direct observation of T Tauri stars inside dark clouds and OB stars in star-forming regions match this
Molecular_cloud
Hot, luminous star with a spectral type of A9 or earlier
type B2Ia Omicron² Canis Majoris, B-type supergiant, spectral type B3Ia Lambda Cephei, O-type supergiant, spectral type O6.5I(n)fp Mu Sagittarii, B-type
Blue_supergiant
Gravitational process studied in astronomy
emission from main-sequence stars. The earliest detections of X-rays from T Tauri stars were made by the Einstein X-ray Observatory. For low-mass stars X-rays
Star_formation
Grouping of evolved cool luminous stars
evolved stars with the Goldreich-Kylafis effect: CARMA observations at $\lambda 1.3$ mm of R Crt and R Leo". The Astrophysical Journal. 899 (2): 152. arXiv:2007
Asymptotic_giant_branch
Process by which stars are named
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Stellar designations and names
Stellar_designations_and_names
Hypothetical compact star
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Q_star
Study of oscillations in stars
globule Young stellar object Protostar Pre-main-sequence Herbig Ae/Be T Tauri Herbig–Haro object Hayashi track Henyey track Evolution Main sequence Red-giant
Asteroseismology
Clustering of stars in astronomy diagram
to be a red-clump star. Other well-known examples include: Capella Aa ε Tauri β Ceti α Cassiopeiae δ Andromedae Arcturus has sometimes been thought to
Red_clump
LAMBDA TAURI
LAMBDA TAURI
Girl/Female
Arabic, Indian, Muslim, Pashtun, Sanskrit
Flame; Large; Spacious; Tall; Another Name for Durga and Lakshmi
Female
Italian
Italian form of English Amber, AMBRA means "amber."
Surname or Lastname
English
English : habitational name from Lambden in Berwickshire.
Girl/Female
Muslim
Dark lipped
Girl/Female
Indian
Flame
Girl/Female
Indian
Praiseworthy, Praiser of Allah
Female
Greek
(Λαμία) Greek myth name of an evil spirit who abducts and devours children, LAMIA means "large shark." The name means "vampire" in Latin and "fiend" in Arabic.
Female
Spanish
Feminine form of Spanish Amado, AMADA means "beloved."
Girl/Female
Muslim
Flame
Girl/Female
Muslim
Praiseworthy, Praiser of Allah
Surname or Lastname
English
English : from a pet form of Lamb 1 and 2.English : from an Old Norse personal name Lambi, from lamb ‘lamb’.
Girl/Female
Muslim
Ambitious
Girl/Female
Indian
Dark lipped
Boy/Male
Hindu
Lord Ganesh, The huge bellied Lord
Girl/Female
Indian
Soft to touch
Girl/Female
Muslim
Soft to touch
Female
Native American
Native American Indian name ALAMEDA means "grove of cottonwood."
Boy/Male
Indian
Jaws.
Girl/Female
Indian
Ambitious
Surname or Lastname
English
English : from Middle English lamb, a nickname for a meek and inoffensive person, or a metonymic occupational name for a keeper of lambs. See also Lamm.English : from a short form of the personal name Lambert.Irish : reduced Anglicized form of Gaelic Ó Luain (see Lane 3). MacLysaght comments: ‘The form Lamb(e), which results from a more than usually absurd pseudo-translation (uan ‘lamb’), is now much more numerous than O’Loan itself.’Possibly also a translation of French agneau.
LAMBDA TAURI
LAMBDA TAURI
Boy/Male
Hindu, Indian, Kannada, Tamil
Follower of Right Way
Girl/Female
Hindu, Indian, Marathi, Sanskrit
Sufficiency
Surname or Lastname
English
English : habitational name from Berkeley in Gloucestershire, named in Old English with be(o)rc ‘birch’ + lēah ‘woodland clearing’. Compare Scottish Barclay.Jewish (American) : assimilated form of Berkowitz.
Girl/Female
Arabic, Islamic
Beautiful and Attractive Lady
Girl/Female
Hindu, Indian, Marathi
Point; Intelligent
Boy/Male
Dutch, German, Scandinavian
The German; From the Netherlands; From Germany
Girl/Female
Hindu, Indian, Malayalam, Marathi
Deer's Eye
Boy/Male
Indian, Punjabi, Sikh
Victorious of the Right
Boy/Male
Arabic, Muslim
Balance of the Most Merciful Allah
Girl/Female
Tamil
Jasodhara | ஜ஼ஸோதரா
(Mother of Lord Buddha)
LAMBDA TAURI
LAMBDA TAURI
LAMBDA TAURI
LAMBDA TAURI
LAMBDA TAURI
n.
A thin plate or scale; a layer or coat lying over another; -- said of thin plates or platelike substances, as of bone or minerals.
a.
Shaped like the Greek letter lambda (/); as, the lambdoid suture between the occipital and parietal bones of the skull.
n.
A monster capable of assuming a woman's form, who was said to devour human beings or suck their blood; a vampire; a sorceress; a witch.
pl.
of Lamina
n.
The point of junction of the sagittal and lambdoid sutures of the skull.
n.
The name of the Greek letter /, /, corresponding with the English letter L, l.
n.
The lamb's-quarters (Chenopodium album).
n.
A thin plate or lamina.
n.
A viola da gamba.
n.
The blade of a leaf; the broad, expanded portion of a petal or sepal of a flower.
n.
A lamb.
imp. & p. p.
of Lamb
n.
A thin plate or scale; specif., one of the thin, flat processes composing the vane of a feather.
n.
A lamb.
v. i.
To bring forth a lamb or lambs, as sheep.
p. pr. & vb. n.
of Lamb
n.
Any person who is as innocent or gentle as a lamb.
pl.
of Lamina
a.
Lamed; lame; disabled; impeded.
n.
A lamp or candlestick.