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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
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-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
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
Gamma-ray Binary in the Large Magellanic Cloud
low-metallicity environments. LMC P3 was initially identified as a high-mass X-ray binary (HMXB) in 2012 through observations with NASA's Chandra X-ray Observatory
LMC_P3
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
Distant star or star cluster
Lensed Star 1, also known as Icarus, at a comoving distance of 14.4 billion light-years (4.4 billion parsecs), was discovered by Hubble in 2018. However, further
Earendel (astronomical object)
Earendel_(astronomical_object)
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
Microlensing event in the constellation Andromeda
Bibcode:2012mgm..conf.2191I. doi:10.1142/9789814374552_0433. ISBN 978-981-4374-51-4. An, Jin H.; Evans, N. W.; Kerins, E.; Baillon, P.; Calchi Novati, S.; Carr
PA-99-N2
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
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
Binary star in the constellation Dorado
torus and the mystery surrounding LMC red supergiant WOH G64". Proceedings of the International Astronomical Union. 4: 454–458. Bibcode:2009IAUS..256.
WOH_G64
Goldilocks terrestrial planet orbiting TOI-700
Alton; Quinn, Samuel N.; Eastman, Jason D.; Cloutier, Ryan; Huang, Chelsea X. (3 January 2020). "The First Habitable Zone Earth-Sized Planet from TESS
TOI-700_d
magnetic field in universe directly detected by X-ray space observatory". phys.org. "Ultra-bright X-ray source awakens near a galaxy not so far away"
List_of_X-ray_pulsars
X-ray binary in Galaxy NGC 300
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 has a mass of 26+7 −5 M☉. Both objects
NGC_300_X-1
Supernova remnant in the constellation Dorado
P.; Harvey, E. (October 2010). "Towards an explanation for the 30 Dor (LMC) Honeycomb nebula - the impact of recent observations and spectral analysis"
Honeycomb_Nebula
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
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
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
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 Triangulum 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
Romano's_Star
Star in the Sunburst galaxy
as measured by MUSE and X-shooter at the Very Large Telescope (VLT) can be quantitatively explained as that of a star cluster 4-6 Myr after formation and
Godzilla_(star)
Supernova in the constellation Dorado
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
Sanduleak_−69_202
Pair of runaway stars in the constellation Libra
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
HD_134439_and_HD_134440
Candidate Thorne–Żytkow object in the constellation Tucana
772 K: ( 5 , 772 3 , 450 ) 4 ⋅ 81 , 283 = 800 R ⊙ . {\displaystyle {\sqrt {{\biggl (}{\frac {5,772}{3,450}}{\biggr )}^{4}\cdot 81,283}}=800\ R_{\odot
HV_11417
Star in the constellation Dorado
stars are not expected to harbor a magnetic dynamo needed to power X-ray emission, an X-ray flux of 3.6×1027 erg/s has been detected at these coordinates
Delta_Doradus
Binary black hole-star systems in the constellation Triangulum
Observing Run". Physical Review X. 13 (4) 041039. arXiv:2111.03606. Bibcode:2023PhRvX..13d1039A. doi:10.1103/PhysRevX.13.041039. "Heaviest Stellar mass
M33_X-7
Contact binary star system in the constellation Dorado
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
VFTS_352
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
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
Coronae Borealis Stars in the Large Magellanic Cloud". Acta Astronomica. 59 (4): 335. arXiv:0912.2097. Bibcode:2009AcA....59..335S. Evans, D. S. (1967).
W_Mensae
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
Red dwarf in the constellation Dorado
Alton; Quinn, Samuel N.; Eastman, Jason D.; Cloutier, Ryan; Huang, Chelsea X. (3 January 2020). "The First Habitable Zone Earth-Sized Planet From TESS
TOI-700
Star in the Triangulum Galaxy
very luminous star. The absolute visual magnitude was estimated to be -9.4, making it brighter than any other blue supergiant. Later in 1990 and 1996
B324
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
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
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
Luminous blue variable star in the constellation Andromeda
Region of the Andromeda Nebula". Harvard College Observatory Bulletin. 851: 4. Bibcode:1927BHarO.851R...4L. Luyten, W. J. (1928). "A New Variable in the
AF_Andromedae
Blue supergiant star in the constellation Leo
49; comoving distance of 14.4 billion light-years; lookback time of 9.34 billion years). Light from the star was emitted 4.4 billion years after the Big
Icarus_(star)
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
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 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
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
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 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
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 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
in LMC; high-mass X-ray binary BI 253 05h 37m 34.46s −69° 01′ 10.2″ 13.88 160000 O2V(f*) in LMC; O2 spectral type standard; runaway star LMC X-4 05h
List_of_stars_in_Dorado
Star in the Small Magellanic Cloud in the constellation Tucana
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
HV_11423
Star in the constellation of Triangulum
temperature of 5,772 K: ( 5 , 772 / 30 , 000 ) 4 ∗ 4 , 680 , 000 = 80 R ⊙ {\displaystyle {\sqrt {(5,772/30,000)^{4}*4,680,000}}=80\ R_{\odot }} Applying the
M33-013406.63
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
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)
X-ray source that only emits soft X-rays
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 binary
Supersoft_X-ray_source
Massive blue supergiant star in the constellation Dorado
arXiv:1105.4757. Bibcode:2011MNRAS.416.1311C. doi:10.1111/j.1365-2966.2011.19129.x. S2CID 118455138. Bestenlehner, J. M.; Gräfener, G.; Vink, J. S.; Najarro
Melnick_42
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
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
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
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 binary star in the constellation Dorado
Variations of Interstellar Depletions and Dust-to-gas Ratio within the LMC". The Astrophysical Journal. 910 (2): 95. arXiv:2101.09399. Bibcode:2021ApJ
HD_38282
Star in the constellation Andromeda
16.2 and 17.6, with very similar V magnitudes, and U magnitudes around 0.4 brighter. The first detailed spectrum was published in 1975. AE And is seen
AE_Andromedae
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
Star in the constellation Dorado
335–340, Bibcode:2009MNRAS.397..335Z, doi:10.1111/j.1365-2966.2009.14917.x. De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor
Theta_Doradus
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 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
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
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
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
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
year. It is strongly suspected to be a binary, due to the detection of hard x-ray emission typical of colliding wind binaries, but the companion is thought
R136c
Triple star system in the constellation Tucana
1088/0004-6256/139/6/2600. hdl:11336/9583. Nazé, Y.; et al. (November 2002). "An X-Ray Investigation of the NGC 346 Field in the Small Magellanic Cloud I. The
HD_5980
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)
Star in the constellation Sagittarius
6822 during a survey of NGC 6822 and IC 1613. In a follow-up study, only 4 of the WR candidates in NGC 6822 were confirmed as WR stars, and they are
NGC_6822-WR_12
Star in the constellation Dorado
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.
Epsilon_Doradus
Class of binary stars
Van Den Heuvel, E. P. J (2007). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy and Astrophysics. 469
X-ray_binary
"On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7". Publications of the Astronomical Society of Japan. 76 (4): 702–707
List_of_smallest_known_stars
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
Wolf-Rayet star in the galaxy IC 1613
"Oxygen and carbon abundances for the WO stars". Space Science Reviews. 66 (1–4): 277–280. doi:10.1007/BF00771077. ISSN 0038-6308. Armandroff, T. E.; Massey
DR1_(star)
Binary star in the Large Magellanic Cloud
heartbeat system in the LMC characterized using ASAS-SN and TESS". Monthly Notices of the Royal Astronomical Society. 489 (4): 4705–4711. arXiv:1901.00005
MACHO_80.7443.1718
Compilation album series
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 2am Remix) 4:38 Rezidents* –
Clubland_X-Treme_Hardcore
of O-type stars by their distance from Earth. The Large Magellanic Cloud (LMC) is around 163 kly distant and the Small Magellanic Cloud (SMC) is around
List_of_O-type_stars
Star in the constellation Dorado
arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976. Gontcharov, G. A. (November 2012), "Spatial distribution
Nu_Doradus
Binary star in the constellation Circinus
Van Den Heuvel, E. P. J (2007). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy & Astrophysics. 469
Circinus_X-1
Astronomical Society. 479 (4): 5101–5123. arXiv:1707.08230. doi:10.1093/mnras/sty1713. ISSN 0035-8711. "Supernova Remnant LMC N132D - NASA Science". 2009-09-09
List_of_supernova_remnants
Astronomical objects
CXJ0110-7211 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
List_of_neutron_stars
Astronomical X-ray source
E. P. J. van den (2007-07-01). "A catalogue of low-mass X-ray binaries in the Galaxy, LMC, and SMC (Fourth edition)". Astronomy & Astrophysics. 469
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
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
Black hole formed by a collapsed star
Stella, L. (1 March 2001). "Broadband X-Ray Spectra of the Persistent Black Hole Candidates LMC X-1 and LMC X-3". The Astrophysical Journal Supplement
Stellar_black_hole
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
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 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
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
British car brand
dormant. Despite being first absorbed by the Leyland Motor Corporation (LMC) in 1966 and a subsequent succession of mergers, nationalisation, and demergers
Rover_(marque)
Interstellar absorption and scattering of light
the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). In the LMC, there is significant variation in the characteristics of the ultraviolet
Extinction_(astronomy)
Outlaw motorcycle club
The Loners Motorcycle Club (LMC) is an international outlaw motorcycle club founded in Woodbridge, Ontario, Canada in 1979. It has seventeen chapters
Loners_Motorcycle_Club
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
restrictive than the LMC since it assumes that each basic covariance k q ( x , x ′ ) {\displaystyle k_{q}(\mathbf {x} ,\mathbf {x} ')} contributes equally
Kernel methods for vector output
Kernel_methods_for_vector_output
LMC X-4
LMC X-4
LMC X-4
LMC X-4
LMC X-4
LMC X-4
LMC X-4
LMC X-4
LMC X-4