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Binary star located in the Small Magellanic Cloud in the constellation Hydrus
AB8, also known as SMC WR8, is a binary star in the Small Magellanic Cloud (SMC). A Wolf–Rayet star and a main-sequence companion of spectral type O orbit
AB8_(star)
Topics referred to by the same term
AB8 or AB-8 may refer to: Aichi AB-8; see List of aircraft (0-A) AB8 (star) ArenaBowl VIII This disambiguation page lists articles associated with the
AB8
Wolf-Rayet star in the galaxy IC 1613
estimated to occur within 17,000 years. Other extragalactic WO stars: AB8 (star) BAT99-123 LH 41-1042 LMC195-1 List of supernova candidates Roman, Nancy
DR1_(star)
Star in the Sunburst galaxy
Godzilla is a variable star candidate in the Sunburst galaxy at redshift z = 2.37 (or 10.9 billion light years from Earth), observed through the gravitational
Godzilla_(star)
Distant star or star cluster
Earendel, designated WHL0137-LS, is a star cluster or a star located in the constellation of Cetus. Discovered in 2022 with the Hubble Space Telescope
Earendel (astronomical object)
Earendel_(astronomical_object)
Blue supergiant star in the constellation Leo
J1149 LS1) is a blue supergiant star observed through a gravitational lens. It is the seventh most distant individual star to have been detected so far (after
Icarus_(star)
(2013). "On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613". Astronomy & Astrophysics. 559: A72. arXiv:1310.2849. Bibcode:2013A&A
List_of_Wolf–Rayet_stars
Star in the Large Magellanic cloud
R99 (HD 269445) is a star in the Large Magellanic Cloud in the constellation Dorado. It is classified as a possible luminous blue variable and is one of
R99_(star)
Small Magellanic Cloud star in the constellation Tucana
HV 2112 is a cool luminous variable star in the Small Magellanic Cloud. Until 2018, it was considered to be the most likely candidate for a Thorne–Żytkow
HV_2112
Stars sorted by absolute magnitude
apparent magnitude (the brightness as seen from Earth), the distance to each star, and a correction for interstellar extinction. The entries in the list below
List_of_most_luminous_stars
X-ray Binary in the Large Magellanic Cloud
ergs/s. This binary system consist of a neutron star accreating matter from an orbiting low-mass blue star. Its high luminosity is caused because of its
LMC_X-2
Binary star in the constellation Dorado
an extreme red supergiant or red hypergiant that may be the largest known star with a well-defined radius, calculated to be around 1,540 times that of the
WOH_G64
Open cluster in the constrellation Hydrus
602c is a looser grouping 11 arc-minutes to the NE, which includes the WO star AB8. NGC 602 includes many young O and B stars and young stellar objects, with
NGC_602
Star in the Triangulum Galaxy
Romano's Star /roʊˈmɑːnoʊz/ (GR 290) is a luminous blue variable star located in the Messier 33 galaxy in the constellation of Triangulum. Discovered by
Romano's_Star
the stars, making it difficult to determine the physical properties of the star needed to calculate its mass: The surrounding gas interferes with the already
List_of_most_massive_stars
Star in the Triangulum Galaxy
brightest star in the Triangulum Galaxy in terms of apparent magnitude. The star has been first catalogued in 1980 by Humphreys and Sandage. The star was found
B324
Wolf–Rayet star in the constellation Dorado
and luminous star known, at around 291 solar masses (M☉) and around 7.2 million times the Sun's luminosity (L☉). It is a Wolf–Rayet star at the center
R136a1
Hypervelocity star in the constellation Dorado
0437−5439 is a massive, unbound hypervelocity star (HVS), also called HVS3. It is a main sequence B-type star located in the Dorado constellation. It was
HE_0437−5439
X-ray binary in the Whirlpool Galaxy
astronomical units. The primary star, M51-ULS-1 A, is a massive, luminous early to late blue supergiant star. The primary star has a spectral type of B2-8la
M51-ULS-1
X-ray binary in the Large Magellanic Cloud
stellar-mass black hole accreting material from a B-type main-sequence companion star, producing intense X-ray emission via a hot accretion disk. LMC X-3 is one
LMC_X-3
Star in the constellation of Triangulum
M33-013406.63, also known as B416 or UIT301, is a O-type blue evolved supergiant star in the constellation of Triangulum. It is located within the Triangulum Galaxy
M33-013406.63
Wolf–Rayet star in the constellation Dorado
LMC195-1 is a Wolf–Rayet star located in the Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, at WO2 the hottest
LMC195-1
Luminous blue variable star in the constellation Triangulum
500,000 in some estimates), it was described as "the brightest nonstable star in M33" and is one of the most luminous stars known. The brightness varies
Var_83
Binary star in the Large Magellanic cloud
34 (abbreviated to Mk34), also called BAT99-116, is a binary Wolf–Rayet star near R136 in the 30 Doradus complex (also known as the Tarantula Nebula)
Melnick_34
Binary star in the Small Magellanic Cloud in the constellation Tucana
AB7, also known as SMC WR7, is a binary star in the Small Magellanic Cloud. A Wolf–Rayet star and a supergiant companion of spectral type O orbit in a
AB7
Star in the constellation Dorado
is a Wolf–Rayet star in R136, a massive star cluster located in Dorado. It is located near R136a1, the most massive and luminous star known. R136a3 is
R136a3
Star in the Large Magellanic Cloud
R71 (RMC 71, HD 269006) is a star in the Large Magellanic Cloud (LMC) in the constellation Mensa. It is classified as a luminous blue variable and is one
R71_(star)
Star in the constellation Dorado
R136a2 (RMC 136a2) is a Wolf-Rayet star residing near the center of the R136, the central concentration of stars of the large NGC 2070 open cluster in
R136a2
Massive blue supergiant star in the constellation Dorado
Melnick 42 is a massive blue supergiant star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Although it is
Melnick_42
X-ray binary in Galaxy NGC 300
Sculptor. It consists of a stellar-mass black hole orbiting a Wolf–Rayet star (specifically of WN spectral type), making it one of only a few confirmed
NGC_300_X-1
Failed supernova (candidate) in the Andromeda Galaxy
supernova candidate located in the Andromeda Galaxy (M31). It is a massive star observed to have undergone a "silent" collapse directly into a black hole
M31-2014-DS1
Star in the constellation Dorado
VFTS 102 is a star located in the Tarantula Nebula, a star forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The peculiarity
VFTS_102
Star in the constellation Dorado
R136b is a blue supergiant star in the R136 cluster in the Large Magellanic Cloud. It is one of the most massive and most luminous stars known. It is found
R136b
Star in the constellation Dorado
R136c is a likely binary star located in R136, a tight knot of stars at the centre of NGC 2070, an open cluster weighing 450,000 solar masses and containing
R136c
Microlensing event in the constellation Andromeda
possibility for the event is that a star in the disk of M31 gravitationally lensed a red giant also in the disk. The lensing star would have a mass between 0
PA-99-N2
Star in the constellation Sagittarius
NGC 6822-WR 12 is a WN-type Wolf–Rayet star located in the galaxy NGC 6822, about 1.54 million light years away in the constellation of Sagittarius. NGC
NGC_6822-WR_12
Wolf Rayet star in the constellation Dorado
LH 41-1042 is a Wolf–Rayet star located in the Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, the second to be
LH_41-1042
Star in the constellation Dorado
called "star 32". The black hole has a mass of around 11 M☉ and the star has a mass of around 32 M☉ and a radius of 17 R☉. With this radius the star nearly
LMC_X-1
Candidate Thorne–Żytkow object in the constellation Tucana
been reported that HV 11417 may be a foreground halo star. As of Gaia's 3rd data release the star has been measured to have a negative parallax, suggesting
HV_11417
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
Contact binary star system in the constellation Dorado
VFTS 352 is a contact binary star system about 160,000 light years away in the Tarantula Nebula, which is part of the Large Magellanic Cloud. It is the
VFTS_352
Triple star system in the constellation Tucana
HD 5980 is a multiple star system on the outskirts of NGC 346 in the Small Magellanic Cloud (SMC) and is one of the brightest stars in the SMC. HD 5980
HD_5980
about 1.44 solar masses and are accreting matter from a binary companion star. The list includes massive Wolf–Rayet stars, which may become Type Ib/Ic
List_of_supernova_candidates
Variable star in the constrellation Hydrus
γ Hydri, Latinised as Gamma Hydri, is a solitary, red-hued star in the constellation Hydrus. It has an apparent visual magnitude of 3.26, making it easily
Gamma_Hydri
Star in the Small Magellanic Cloud in the constellation Tucana
HV 11423 (PMMR 114 or 140 LI-SMC) is a red supergiant star in the Small Magellanic Cloud. It is about 200,000 light-years away towards the constellation
HV_11423
High-mass X-ray binary
It corresponds to a high-mass X-ray binary in which the normal star is a Wolf–Rayet star and the compact object is a stellar black hole. The mass of this
IC_10_X-1
Variable star in the Large Magellanic Cloud
binary and Cepheid variable star, pulsating every 3.8 days. The star, in the Large Magellanic Cloud, was the first Cepheid star system found to be orbiting
OGLE-LMC-CEP0227
Star in the constellation Dorado
brightest stars in the Large Magellanic Cloud (LMC). It is a suspected variable star. HD 33579 lies in a part of the Hertzsprung–Russell diagram referred to as
HD_33579
An O-type star is a hot, blue star of spectral type O in the Yerkes classification system employed by astronomers. They have surface temperatures in excess
List_of_O-type_stars
Star in the constellation Dorado
HD 269810 is a blue giant star in the Large Magellanic Cloud. It is one of the most massive and most luminous stars known, and one of only a handful of
HD_269810
Binary black hole-star systems in the constellation Triangulum
Galaxy. The system is made up of a stellar-mass black hole and a companion star. The black hole in M33 X-7 has an estimated mass of 15.65 times that of the
M33_X-7
Pair of runaway stars in the constellation Libra
are roughly 96 ly away, they have one of the highest proper motions of any star in the sky, travelling over 3.5 arcseconds every year. The stars are believed
HD_134439_and_HD_134440
X-ray binary in the Large Magellanic Cloud
neutron star and a massive companion star, exhibiting periodic X-ray eclipses and long-term intensity variations. LMC X-4 comprises a neutron star with a
LMC_X-4
Wolf-Rayet star in the constellation Dorado
1970, and identified as a star with strong OVI emission in 1971, alongside other WO stars like WR 102, WR 142 and SMC AB8. Most stars with strong OVI
BAT99-123
Star in the constellation Dorado
BAT99-98 is a Wolf–Rayet star located in the Large Magellanic Cloud, in NGC 2070 near the R136 cluster in the Tarantula Nebula (30 Doradus). At estimates
BAT99-98
Binary star in the Large Magellanic Cloud
MACHO 80.7443.1718 is a binary star in the LH 58 association in the Large Magellanic Cloud, in the constellation of Dorado, first identified among about
MACHO_80.7443.1718
Supernova in the constellation Dorado
supergiant star, located on the outskirts of the Tarantula Nebula in the Large Magellanic Cloud. It was the progenitor of supernova 1987A. The star was originally
Sanduleak_−69_202
O-type main sequence star in the constellation Dorado
BI 253 is an O2V star in the Large Magellanic Cloud and is a primary standard of the O2 type. It is one of the hottest main-sequence stars known and one
BI_253
Wolf Rayet star in the constellation Dorado
VFTS 682 is a Wolf–Rayet star in the Large Magellanic Cloud. It is located over 29 parsecs (95 ly) north-east of the massive cluster R136 in the Tarantula
VFTS_682
Star in Large Magellanic Cloud
Large Magellanic Cloud and one of the brightest stars in its galaxy. The star was first mentioned in a 1901 paper as an object with an unusual spectrum
HD_37836
Star in the constellation Andromeda
variable (LBV), a type of variable star. The star is one of the most luminous variables in M31, the Andromeda Galaxy. The star was discovered to be variable
AE_Andromedae
Binary star in the constellation Dorado
R145 (HD 269928) is a spectroscopic binary star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Both components
R145
List of the hottest known stars
luminous stars List of least massive stars List of coolest stars "Wolf-Rayet Star Catalogue". pacrowther.staff.shef.ac.uk. Retrieved 2021-05-28. Sander, A
List_of_hottest_stars
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. It is
IRAS_05280−6910
System for identifying vehicles
Yugoslavia/Serbia Zastava Automobiles V31 Croatia Tvornica Autobusa Zagreb (TAZ) V39 AB8 Rimac Automobili WAC Germany Audi/Porsche RS 2 Avant WAG Neoplan WAU Audi
Vehicle_identification_number
Massive binary star in the constellation Dorado
HD 38282 (R144, BAT99-118, Brey 89) is a massive spectroscopic binary star in the Tarantula Nebula (Large Magellanic Cloud), consisting of two hydrogen-rich
HD_38282
Luminous blue variable star in the constellation Andromeda
variable (LBV), a type of variable star. The star is one of the most luminous variables in M31, the Andromeda Galaxy. The star was discovered to be variable
AF_Andromedae
Star in the constellation Dorado
arcseconds. The direction of the source corresponded with the remnants of a star that had gone supernova around 3000 B.C.E. The event was named GRB 790305b
SGR_0526−66
Neutron star
compact object in this system has been unambiguously identified as a neutron star with a spin period of 3 seconds. The Swift BAT all-sky survey detected hard
3XMM_J004232.1+411314
Star in the constellation Dorado
LH 54-425 is a spectroscopic binary star system in the LH 54 OB association within the Large Magellanic Cloud in the constellation Dorado. The OB association
LH_54-425
Pulsar in the constellation Dorado
Small Magellanic Cloud AB7 AB8 HD 5980 HV 2112 HV 11417 HV 11423 Triangulum Galaxy B324 M33 X-7 M33-013406.63 Romano's Star Var 83 Other DR1 Earendel Godzilla
PSR_J0540−6919
Star in the constellation Dorado
RMC (Radcliffe observatory Magellanic Cloud) 126, is a massive luminous star with several unusual properties. It exhibits the B[e] phenomenon where forbidden
HD_37974
Star in the constellation Hydrus
Eta1 Hydri, Latinized from η1 Hydri, is a blue-white hued star in the southern constellation of Hydrus. It has an apparent visual magnitude of 6.76, which
Eta1_Hydri
Star in the Large Magellanic Cloud
satellite galaxy of the Milky Way, located roughly 160,000 light-years away. The star is a luminous blue variable, and one of the most luminous stars known, having
S_Doradus
Possible red cataclysmic variable star in the constellation Andromeda
M31 RV is a possible red cataclysmic variable star located in the Andromeda Galaxy (M31) that experienced an outburst in 1988, which was similar to the
M31_RV
Star in the constellation Hydrus
Theta Hydri, Latinized from θ Hydri, is a blue-white hued star in the southern constellation of Hydrus. It is faintly visible to the naked eye with an
Theta_Hydri
Variable star in the constellation Mensa
W Mensae (W Men) is an unusual yellow supergiant star in the Large Magellanic Cloud in the southern constellation Mensa. It is an R Coronae Borealis variable
W_Mensae
Yellow hypergiant in the Large Magellanic Cloud
163,000 ly), the star is observable through a small telescope due to its immense luminosity, at an apparent magnitude of 9.6. The star is extremely luminous
HD_271182
Candidate luminous variable star in the constellation Dorado
Small Magellanic Cloud AB7 AB8 HD 5980 HV 2112 HV 11417 HV 11423 Triangulum Galaxy B324 M33 X-7 M33-013406.63 Romano's Star Var 83 Other DR1 Earendel Godzilla
R85
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