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X-ray Binary in the Large Magellanic Cloud
LMC X-2 is a low-mass X-ray binary (LMXB) located in the Large Magellanic Cloud (LMC), a satellite galaxy of Milky Way. It is one of the five brightest
LMC_X-2
Star in the constellation Dorado
LMC X-1 is the first X-ray source detected in the Large Magellanic Cloud. It was discovered in 1969, using data from an instrument carried by a Sandia
LMC_X-1
X-ray binary in the Large Magellanic Cloud
LMC X-4 is an eclipsing high-mass X-ray binary (HMXB) pulsar system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately
LMC_X-4
X-ray binary in the Large Magellanic Cloud
LMC X-3 is a high-mass X-ray binary (HMXB) system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately 165,000
LMC_X-3
Satellite galaxy of the Milky Way
Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (163,000 light-years), the LMC is the second-
Large_Magellanic_Cloud
Gamma-ray Binary in the Large Magellanic Cloud
LMC P3 (also known as 4FGL J0535.2-6736) is a gamma-ray binary star system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky
LMC_P3
Distant star or star cluster
900 million years after the Big Bang. The star has been determined to have a 6.2±0.1 redshift, meaning the light from Earendel reached Earth 12.9 billion years
Earendel (astronomical object)
Earendel_(astronomical_object)
Star in the constellation Dorado
one of which was Mel J. It was numbered 12, and referred to as AB12, or LMC AB12 to distinguish it from the better-known AB stars in the Small Magellanic
BAT99-98
Wolf–Rayet star in the constellation Dorado
the brightness and spectra of bright stars in the Large Magellanic Cloud (LMC). Among the objects cataloged was RMC 136 (Radcliffe observatory Magellanic
R136a1
Binary star in the constellation Dorado
M. (July 2008). "Resolving the dusty torus and the mystery surrounding LMC red supergiant WOH G64". Proceedings of the International Astronomical Union
WOH_G64
X-ray binary in Galaxy NGC 300
(designated #41 in NGC 300), yielding an orbital period of 32.3±0.2 h, consistent with the X-ray period. The black hole has a mass of 17±4 M☉ and the WR star
NGC_300_X-1
X-ray binary in the Whirlpool Galaxy
M51-ULS-1, also known as RX J132943+47115, is a high-mass X-ray binary (HMXB) system in the constellation of Canes Venatici. The binary system is located
M51-ULS-1
Astrometric binary star system in the constellation Mensa
Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. de Bruijne
Gamma_Mensae
Microlensing event in the constellation Andromeda
exoplanet could be confirmed, it would be the most distant known planet, 2.58 Million ly away.) "MEGA-ML 7". SIMBAD. Centre de données astronomiques
PA-99-N2
Failed supernova (candidate) in the Andromeda Galaxy
05280−6910 LH 41-1042 LH 54-425 LMC P3 LMC X-1 LMC X-2 LMC X-3 LMC X-4 LMC195-1 MACHO 80.7443.1718 Melnick 34 Melnick 42 OGLE-LMC-CEP0227 PSR J0523−7125 PSR
M31-2014-DS1
Variable star in the Large Magellanic Cloud
OGLE-LMC-CEP0227 is an eclipsing binary and Cepheid variable star, pulsating every 3.8 days. The star, in the Large Magellanic Cloud, was the first Cepheid
OGLE-LMC-CEP0227
High-mass X-ray binary
IC 10 X-1 is an X-ray source located in the dwarf galaxy IC 10, an irregular galaxy. It corresponds to a high-mass X-ray binary in which the normal star
IC_10_X-1
Star in the constellation Mensa
the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
Beta_Mensae
Star in the constellation Mensa
Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Koen, Chris;
Xi_Mensae
Binary black hole-star systems in the constellation Triangulum
M33 X-7 is a black hole binary system in the Triangulum Galaxy. The system is made up of a stellar-mass black hole and a companion star. The black hole
M33_X-7
Red supergiant star in the Large Magellanic Cloud
IRAS 05280−6910 (LI-LMC 1100 or NGC 1984-IRS1) is an extreme red supergiant star located in the Large Magellanic Cloud and the open cluster NGC 1984.
IRAS_05280−6910
Star in the constellation Dorado
et al. (January 2015). "The evolution of rotating very massive stars with LMC composition". Astronomy & Astrophysics. 573: A71. arXiv:1501.03794. Bibcode:2015A&A
HD_269810
Luminous blue variable star in the constellation Triangulum
arXiv:0903.5222. Bibcode:2009MNRAS.396L..21V. doi:10.1111/j.1745-3933.2009.00654.x. S2CID 14666975. Van Den Bergh, S.; Herbst, E.; Kowal, C. T. (1975). "A survey
Var_83
O-type main sequence star in the constellation Dorado
Mianes, P.; Prévot, L.; Rebeirot, E.; Rousseau, J. (1975). "Studies of the LMC stellar content. I. A catalogue of 272 new O-B2 stars". Astronomy and Astrophysics
BI_253
Candidate Thorne–Żytkow object in the constellation Tucana
Their Luminosity Functions in M31 and M33". The Astrophysical Journal. 942 (2): 69. arXiv:2211.14147. Bibcode:2023ApJ...942...69M. doi:10.3847/1538-4357/aca665
HV_11417
Star in the Sunburst galaxy
source-frame ultraviolet light and nebular emission lines as measured by MUSE and X-shooter at the Very Large Telescope (VLT) can be quantitatively explained
Godzilla_(star)
Contact binary star system in the constellation Dorado
The Astrophysical Journal. 812 (2): 102. arXiv:1509.08940. Bibcode:2015ApJ...812..102A. doi:10.1088/0004-637X/812/2/102. S2CID 53653307. "Final Kiss
VFTS_352
Pair of runaway stars in the constellation Libra
Research Notes of the American Astronomical Society. 2 (2): 45. arXiv:1806.00049. Bibcode:2018RNAAS...2...45D. doi:10.3847/2515-5172/aac94f. Chen, Yu; King
HD_134439_and_HD_134440
Supernova in the constellation Dorado
the invention of the telescope, when its maximum reached visual magnitude +2.8. The discovery that a blue supergiant was a supernova progenitor contradicted
Sanduleak_−69_202
Star in the constellation Dorado
B0565−66) is a soft gamma repeater (SGR), located in the supernova remnant LMC N49, in the Large Magellanic Cloud. It was the first soft gamma repeater
SGR_0526−66
Star in the constellation Mensa
Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Eggen, Olin
Zeta_Mensae
Star in the constellation Mensa
Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Brown, A.
Eta_Mensae
Hypervelocity star in the constellation Dorado
2007.00280.x. S2CID 2992585. Przybilla, N.; Nieva, M. F.; Heber, U.; Firnstein, M.; Butler, K.; Napiwotzki, R.; Edelmann, H. (2008). "LMC origin of the
HE_0437−5439
Star in the Triangulum Galaxy
in the Triangulum Galaxy, located near the giant H II region IC 142 around 2.7 million light years away. It is the brightest star in the Triangulum Galaxy
B324
Supernova remnant in the constellation Dorado
a massive burst of Gamma-ray and X-ray emissions from LMC N49 , confirmed to be particularly strong by the first X-ray telescope, the Einstein Observatory
LMC_N49
Star in Large Magellanic Cloud
unusual spectrum with bright H-alpha, H-beta and H-delta lines located in the LMC. Later it was catalogued in the Henry Draper Catalogue and given the designation
HD_37836
Variable star in the constellation Mensa
Notices of the Royal Astronomical Society. 268 (2): 544. Bibcode:1994MNRAS.268..544P. doi:10.1093/mnras/268.2.544. Luyten, W. J. (1927). "A New Irregular
W_Mensae
Pulsar in the constellation Dorado
R. P.; Sartori, A.; et al. (June 2010). "HST/WFPC2 observations of the LMC pulsar PSR B0540-69". Astronomy and Astrophysics. 515: A110. arXiv:1003.0786
PSR_J0540−6919
Star in the Triangulum Galaxy
nature of Romano's star (GR 290) in M 33". Astronomy and Astrophysics. 411 (2): 193. Bibcode:2003A&A...411..193P. doi:10.1051/0004-6361:20031149. Maryeva
Romano's_Star
Star in the constellation of Triangulum
772 K: ( 5 , 772 / 10 , 000 ) 4 ∗ 10 5.6 = 210.2 R ⊙ {\displaystyle {\sqrt {(5,772/10,000)^{4}*10^{5.6}}}=210.2\ R_{\odot }} Van Leeuwen, F. (2007). "Validation
M33-013406.63
Star in the constellation Dorado
supergiants S 18 in the SMC and R 66 = HDE 268835 and R 126 = HD 37974 in the LMC". Astronomy and Astrophysics. 386 (3): 926. Bibcode:2002A&A...386..926V.
HD_37974
X-ray source that only emits soft X-rays
(MW halo near LMC), RX J0513.9-6951 (LMC), RX J0527.8-6954 (LMC), RX J0537.7-7034 (LMC), CAL 83 (LMC), CAL 87 LMC), and 1E 0035.4-7230 (SMC). A symbiotic
Supersoft_X-ray_source
Star in the constellation Dorado
hypergiant and one of the brightest stars in the Large Magellanic Cloud (LMC). It is a suspected variable star. HD 33579 lies in a part of the Hertzsprung–Russell
HD_33579
Candidate luminous variable star in the constellation Dorado
(1998). "Light variations of massive stars (alpha Cyg variables). XVI. The LMC supergiants R 85 (LBV) and R 110 (LBV) and the SMC supergiants R 42 and R
R85
Massive binary star in the constellation Dorado
Interstellar Depletions and Dust-to-gas Ratio within the LMC". The Astrophysical Journal. 910 (2): 95. arXiv:2101.09399. Bibcode:2021ApJ...910...95R. doi:10
HD_38282
Luminous blue variable star in the constellation Andromeda
as one of the five Hubble–Sandage variables: Var A, Var B, Var C, and Var 2 in M33, and Var 19 in M31. On the basis of color–color comparisons, it was
AF_Andromedae
Binary star located in the Small Magellanic Cloud in the constellation Hydrus
been detected as an x-ray source. This is unexpected because close pairs of hot luminous stars are expected to produce copious x-ray emission from colliding
AB8_(star)
Wolf Rayet star in the constellation Dorado
et al. (January 2015). "The evolution of rotating very massive stars with LMC composition". Astronomy & Astrophysics. 573: A71. arXiv:1501.03794. Bibcode:2015A&A
VFTS_682
Massive blue supergiant star in the constellation Dorado
Royal Astronomical Society. 416 (2): 1311. arXiv:1105.4757. Bibcode:2011MNRAS.416.1311C. doi:10.1111/j.1365-2966.2011.19129.x. S2CID 118455138. Bestenlehner
Melnick_42
Blue supergiant star in the constellation Leo
so far (after Earendel, Godzilla, Mothra, Quyllur, MACS J0647.7+7015 LS1 & 2), at approximately 14 billion light-years from Earth (redshift z=1.49; comoving
Icarus_(star)
Star in the constellation Mensa
emission features in the spectrum. It is young star and an X-ray source, one of the brightest such X-ray emitters in the solar neighborhood, and is categorized
AO_Mensae
Wolf–Rayet star in the constellation Dorado
Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, at WO2 the hottest known in the LMC. It is likely to be one of
LMC195-1
Possible red cataclysmic variable star in the constellation Andromeda
1054–1056. Bibcode:2003MNRAS.343.1054E. doi:10.1046/j.1365-8711.2003.06755.x. ISSN 0035-8711. Rich, R. Michael; Mould, Jeremy; Picard, Alain; Frogel, Jay
M31_RV
Star in the constellation Dorado
R136a2 is challenging due to many factors. At the immense distance to the LMC, the parallax method is beyond the limits of current technology. Most estimates
R136a2
V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 2007-01-04. Gould, B. A. "Uranometria Argentina". Reprinted and
List_of_stars_in_Mensa
Small Magellanic Cloud star in the constellation Tucana
S.; Zu, Y.; Peterson, B. M.; et al. (2014). "The Man behind the Curtain: X-Rays Drive the UV through NIR Variability in the 2013 Active Galactic Nucleus
HV_2112
Neutron star
3XMM J004232.1+411314 is a low-mass X-ray binary hosted in the galaxy M31. It is the most luminous source of hard X-rays in the Andromeda Galaxy. It is
3XMM_J004232.1+411314
Binary star in the Small Magellanic Cloud in the constellation Tucana
expected to be, and are observed to be, weaker than in galactic and LMC WR stars, the X-ray luminosity is comparable to similar galactic binaries. Auger
AB7
Star in the Large Magellanic Cloud
Magellanic Cloud (LMC) in the constellation Mensa. It is classified as a luminous blue variable and is one of the most luminous stars in the LMC. It lies three
R71_(star)
Star in the Large Magellanic cloud
(1998). "Light variations of massive stars (alpha Cyg variables). XV. The LMC supergiants R99 (LBV), R103, R123 (LBV) and R128". Astronomy and Astrophysics
R99_(star)
Surface analytical technique
J.G.; Buydens, L.M.C. (1998). "Application of genetic algorithms for characterization of thin layered materials by glancing incidence X-ray reflectometry"
X-ray_reflectivity
Star in the constellation Dorado
of the Royal Astronomical Society. 408 (2): 731. arXiv:1007.3284. Bibcode:2010MNRAS.408..731C. doi:10.1111/j.1365-2966.2010.17167.x. S2CID 53001712.
R136b
Star in the constellation Dorado
VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?". The Astrophysical Journal
VFTS_102
Star in the Large Magellanic Cloud
known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160,000 light-years
S_Doradus
Class of binary stars
"A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy and Astrophysics. 469 (2): 807. arXiv:0707.0544. Bibcode:2007A&A
X-ray_binary
Binary star in the constellation Dorado
catalogue entry number, or just R with the number. In the first catalogue of LMC Wolf-Rayet stars, R145 is listed as number 90 with spectral type WN7. Stars
R145
Wolf Rayet star in the constellation Dorado
Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, the second to be discovered in the LMC and one of only three found
LH_41-1042
Type of low-mass X-ray binary
X-ray flares. Some Z sources may have constant flares, giving them higher temperatures and nonstop jets. Scorpius X-1 Circinus X-1 LMC X-2 Cygnus X-2
Z_source
Star in the constellation Andromeda
similar to the five Hubble–Sandage variables: Var A, Var B, Var C, and Var 2 in M33, and Var 19 in M31 (=AF Andromedae). On the basis of color–color comparisons
AE_Andromedae
Binary star in the Large Magellanic cloud
shows high x-ray luminosity characteristic of colliding-wind binaries, and periodic variations in luminosity, spectral absorption, and the x-ray brightness
Melnick_34
Star in the constellation Dorado
arXiv:astro-ph/0205028. Bibcode:2002MNRAS.336..309O. doi:10.1046/j.1365-8711.2002.05754.x. S2CID 117980967. Massey, Philip; Morrell, Nidia I.; Neugent, Kathryn F.;
LH_54-425
Compilation album series
Neo Cortex – Elements (KB Project Remix) 3:55 LMC vs U2 – Take Me to the Clouds Above (Lee S Remix) 2:51 Narcotic Thrust – I Like It (Sinewave Surfers
Clubland_X-Treme_Hardcore
Star in the constellation Sagittarius
"Locating Red Supergiants in the Galaxy NGC 6822". The Astronomical Journal. 163 (2): 70. arXiv:2112.03990. Bibcode:2022AJ....163...70D. doi:10.3847/1538-3881/ac410e
NGC_6822-WR_12
Triple star system in the constellation Tucana
the Royal Astronomical Society. 338 (2): 360–388. Bibcode:2003MNRAS.338..360F. doi:10.1046/j.1365-8711.2003.06052.x. Massey, Philip; Olsen, K. A. G.; Parker
HD_5980
Magellanic Cloud (LMC) is around 163 kly distant and the Small Magellanic Cloud (SMC) is around 204 kly distant The Andromeda Galaxy (M31) is 2.5 Mly distant
List_of_O-type_stars
Star in the constellation Mensa
Astronomical Society, 419 (2): 1637–1641, arXiv:1109.4800, Bibcode:2012MNRAS.419.1637L, doi:10.1111/j.1365-2966.2011.19826.x, S2CID 117788450. Houk, Nancy;
Lambda_Mensae
Star in the constellation Dorado
Royal Astronomical Society. 408 (2): 731. arXiv:1007.3284. Bibcode:2010MNRAS.408..731C. doi:10.1111/j.1365-2966.2010.17167.x. S2CID 53001712. Hainich, R.;
R136c
Yellow hypergiant in the Large Magellanic Cloud
variable. It is one of the brightest stars in the Large Magellanic Cloud (LMC), positioned in the deep southern constellation of Dorado. It is receding
HD_271182
Star in the constellation Mensa
the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
Mu_Mensae
Binary star in the Large Magellanic Cloud
(11 November 2019). "An extreme amplitude, massive heartbeat system in the LMC characterized using ASAS-SN and TESS". Monthly Notices of the Royal Astronomical
MACHO_80.7443.1718
Star in the Small Magellanic Cloud in the constellation Tucana
times larger than the sun. It is also a variable star with a variation of up 2 magnitudes at visual wavelengths but essentially constant in the infrared
HV_11423
Wolf-Rayet star in the galaxy IC 1613
This is several hundred million times faster than the Sun's, which is at (2–3)×10−14 M☉ per year. The brightest HII region in IC 1613, S3 was first catalogued
DR1_(star)
Binary star system in the constellation Mensa
Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. van Leeuwen
Delta_Mensae
Black hole formed by a collapsed star
Black Hole in LMC X-3". The Astrophysical Journal. 794 (2): 154. arXiv:1402.0085. Bibcode:2014ApJ...794..154O. doi:10.1088/0004-637X/794/2/154. ISSN 0004-637X
Stellar_black_hole
Star in the constellation Dorado
the Royal Astronomical Society. 408 (2): 731–751. arXiv:1007.3284. Bibcode:2010MNRAS.408..731C. doi:10.1111/j.1365-2966.2010.17167.x. S2CID 53001712.
R136a3
Nebula in the Large Magellanic Cloud
LMC N79 (or LHα 120-N79) is an emission nebula in the Large Magellanic Cloud. The nebula is part of the catalog of H-alpha stars and nebulae by Karl G
LMC_N79
Binary star in the constellation Circinus
(2007). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy & Astrophysics. 469 (2): 807. arXiv:0707.0544. Bibcode:2007A&A
Circinus_X-1
Astronomical objects
Vela X-1 4U 0352+309 Bursting Pulsar Vela Junior LMC N49 Intermediate-mass X-ray binary High-mass X-ray binaries Centaurus X-3 Circinus X-1 GX 301-2 Hercules
List_of_neutron_stars
Astronomical X-ray source
(2007-07-01). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy & Astrophysics. 469 (2): 807–810. arXiv:0707.0544.
Scorpius_X-1
Dwarf irregular galaxy, satellite galaxy of the Milky Way
of interactions between the SMC and LMC. The Small Magellanic Cloud contains a large and active population of X-ray binaries. Recent star formation has
Small_Magellanic_Cloud
arXiv:1707.08230. doi:10.1093/mnras/sty1713. ISSN 0035-8711. "Supernova Remnant LMC N132D - NASA Science". 2009-09-09. Retrieved 2025-09-20. Francis, Reddy.
List_of_supernova_remnants
Type of x-ray binary
(2010). "Optical identification of the transient supersoft X-ray source RX J0527.8-6954, in the LMC". Astronomy and Astrophysics. 517: L5. arXiv:1006.4820
Be–white dwarf X-ray binary system
Be–white_dwarf_X-ray_binary_system
Subfield of astronomy
expanded to cover wavelengths extending from radio waves through optical, x-ray, and gamma wavelengths. In the 21st century, it further expanded to include
Astrophysics
American stock car racing team
Darius Rucker was named co-owner of LMC. On June 25, 2026, Guy Fieri was named strategic owner of LMC. On July 30, 2026, LMC announced that the team would be
Legacy_Motor_Club
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
(R62 in LMC) HD 37974 (R126 in LMC) HD 80077, LBV candidate` HD 268835 (R66 in LMC) HD 269781 (in LMC) HD 269661 (R111 in LMC) HD 269604 (in LMC) HD 269896
Hypergiant
American cyclist (born 1971)
Académie des Sports. "Grand Prix De L'Académie Des Sports – Prix Serge Kampf". LMC France. Archived from the original on May 6, 2012. Retrieved August 27, 2012
Lance_Armstrong
1086/144923. ISSN 0004-637X. Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W.; Brunthaler, A. (2012). "The distance and size of the red hypergiant NML
List_of_largest_stars
Defunct American rubber, related chemicals and rocket manufacturer (1929–2007)
to CTEC and its snow equipment division to Logan Manufacturing Company (LMC), owned by John DeLorean. In 1980, Thiokol acquired Carlisle Chemical Company
Thiokol
Cloud (LMC). When there are often many individually discernible sources, the first one identified is usually designated as the extragalactic source X-1, e
History_of_X-ray_astronomy
Interstellar absorption and scattering of light
ISBN 978-0-691-00402-0. Howarth, I. D. (1983). "LMC and galactic extinction". Monthly Notices of the Royal Astronomical Society. 203 (2): 301–304. Bibcode:1983MNRAS.203
Extinction_(astronomy)
LMC X-2
LMC X-2
Girl/Female
Tamil
Sita, Made of lac
Boy/Male
American, Australian, Aztec, British, Danish, Dutch, English, French, German, Greek, Hebrew, Latin, Swiss
Light; Illumination; Form of Luke; A Region of Southern Italy; Bringer of Light
Male
Hungarian
Hungarian form of Latin Columbanus, KÃLMÃN means "dove."
Boy/Male
Indian, Sanskrit
Silkworm; Lac-insect; Ant
Boy/Male
French Welsh
Light; illumination. Form of Luke.
Surname or Lastname
English
English : occupational name for a locksmith, from an agent derivative of Middle English, Old English loc ‘lock’, ‘fastening’ (see Lock).English : topographic name for someone who lived by a lock or enclosure, from a derivative of Middle English loke (see Lock 2).English : variant of Luker.
Girl/Female
English
Lucky. Can be a names starting with 'Luc-'.
Girl/Female
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sindhi, Telugu
Sita; Made of Lac
Male
Arthurian
, (lake), a king; the father of Erec.
Surname or Lastname
Scottish and English
Scottish and English : variant of Lockhart 1 and 2.English : from Middle English Locward ‘keeper of the fold’, from Old English, Middle English loc ‘enclosure’, ‘fold’ + Middle English ward ‘guardian’, ‘keeper’ (Old English weard)
Male
French
Norman French form of Latin Lucas, LUC means "from Lucania."
Surname or Lastname
English
English : topographic name for someone who lived by a grove or thicket, Middle English grove, Old English grÄf.English (Huguenot) : Americanized spelling of the French surname Le Grou(x) or Le Greux (see Groulx).North German form of Grob.North German : habitational name from any of several places named Grove or Groven in Schleswig-Holstein, which derive their name from Middle Low Germany grÅve ‘ditch’, ‘channel’. In some cases the name is a Dutch or Low German form of Grube.Altered form of German Graf.The surnames Grove and Groves are common mainly in the West Midlands. A Huguenot family who acquired the name Grove are descended from a certain Isaac Le Greux or Grou(x) or his brother. They fled from Tours in France in the late 17th century and settled in Spitalfields, London. Their children were known as Grou(x) or Grove; their grandchildren also used the form Grew; but their great-grandchildren, born at the end of the 18th century, were universally Grove.
Biblical
Search for "List of biblical names starting with X"
in existing articles.
Search for "List of biblical names starting with X"
Female
French
Feminine form of French Luc, LUCE means "from Lucania."
Surname or Lastname
English (mainly Dorset)
English (mainly Dorset) : occupational name for a locksmith, from an agent derivative of Middle English, Old English loc ‘lock’, ‘fastening’ (see Lock, and compare Locker).
Boy/Male
American, Australian, British, English, Vietnamese
Lives by the Stronghold; Luck; Blessings
Male
French
French form of Latin Bartholomaeus, BARTHÉLMY means "son of Talmai."Â
Boy/Male
English
Lives by tbe stronghold.
Surname or Lastname
English
English : habitational name, probably from Lockeridge in Wiltshire, or Lockridge Farm in Devon, both named from Old English loc(a) ‘enclosure’, ‘fold’ (see Lock 2) + hrycg ‘ridge’.
Biblical
to start the List of biblical names starting with X article alternatively use the Article Wizard, or add a request for it.
LMC X-2
LMC X-2
LMC X-2
LMC X-2
LMC X-2
LMC X-2
LMC X-2