List of Wolf-Rayet stars

Last updated

This is a list of Wolf-Rayet stars, in order of their distance from Earth. [1] [2] [3]

Contents

List

Milky Way Galaxy

Star system NebulaMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
Gamma² Velorum (WR 11/Suhail al Muhlif/Regor)1096+26
−23
2WC81.83The Closest Wolf-Rayet star to Earth.
HD 45166 3,2322qWR9.88The primary of HD 45166 is currently the only known example of a qWR star.
HD 112313 3,377.2±153.61WCCenter star of NGC 4361 Nebula.
WR 142 Sadr Region rgb.jpg 4,0001WO212.94
HD 151932 (WR 78)4,1001WN7h6.45 - 6.61
HD 326823 (V1104 Scorpii)4,1421WNpec9.03
HD 151932 (WR 78)4,2001WN7h6.45 - 6.61
EZ Canis Majoris (WR 6) Sh2-308.jpg 4,9001WN4-s6.91
WR 111 (HD 165763)5,316+320
−230
1WC5+7.82
WR 140 (SBC9 1232) WR140.png 5,600 ± 3002WC7p6.85
HD 152408 (WR 79a) The Prawn Nebula in Scorpius.jpg 5,6001WN9ha5.81-5.85
WR 93 5,9001WC7
WR 133 (V1676 Cyg)6,100 ± 3002WN5o6.75 - 6.84
HD 152408 (WR 79a)6,5001WN9ha5.81-5.85
WR 25 (HD 93162) Carina Nebula by ESO.jpg 6,5002O2.5If*/WN68.80
Apep (WR 70-16) The triple star system 2XMM J160050.7-514245 (Apep).jpg 6523+400
−300
3WR + WR
CV Serpentis (WR 113)6,700 ± 2002WC8d9.08
WR 136 (HD 192163) NGC 6888 HOO By Don Christopher Deaver.jpg 6,700 ± 5001WN6(h)-s7.50
WR 86 6849 ± 8001WR9.27
HD 83535 7,2701WC3Central star of NGC 2867 Nebula.
Theta Muscae (WR 48a)7,4004WC5/65.53
WR 93b Antares overlooking an Auxiliary Telescope.jpg 7,600 ± 5001WO315.2
WR 2 8,1861WN2-w11.33
WR 22 (V429 Carinae) Carina Nebula around the Wolf-Rayet star WR 22.jpg 8,300 ± 7002WN7h6.42
WR 104 (V5097 Sgr) Wr104 sslkeck big.jpg 8,4003WC9d13.28 + 15.36
AG Pegasi 9,0002WR6.0 - 9.4
WR 8 9,0001WR
WR 46 (DI Crucis)9,300 ± 9001WN3p-w10.83
WR 3 9,458+520
−390
1WN3-hw10.69
WR 102 9,500 ± 6001WO214.10
WR 138 10,0001WR
WR 1 10,500 ± 5001WN4-s10.54
WR 157 11285.011WN4.5Member of Markarian 50 Cluster.
WR 69 11,3501WC9d9.1
WR 9 12,000 ± 6002WC410.50
WR 142a 13,0001WR
WR 21a 13,100 ± 7001O3/WN5ha + O3Vz((f*))12.661
CD Crucis (WR 47)14,0002WN6o10.81
WR 120–6 14,0001WN4It is the central star of Abell 48 Planetary Nebula.
WR 24 (HD 93131)14,0001WN6ha-w6.48 - 6.50
WR 20a 14,000 ± 1,0002O3If*/WN6 + O3If*/WN613.28
WR 142b 15,0001WR
WR 7 (HD 56925)16,0001WN4-s11.56
AG Carinae 17,000 ± 1,0002WN116.96
WR 12 (V378 Velorum)19,000 ± 1,0001WN8h10.78
OAO 1657-415 20,0001Ofpe/WN9>23
WR 124 (QR Sagittae)21,000 ± 2,0001WN8h11.50±0.11
WR 30a 21,917+1,400
−1,090
1WO4
Cygnus X-3 (WR 145a/V1521 Cyg)24,135±1,1001WN 4–6
NGC 3603-A1 (WR 43a/HD 97950A1)24,8002WN6h+WN6h11.18
NGC 3603-B (WR 43b/HD 97950B)24,8001WN6h11.33
NGC 3603-C (WR 43c/HD 97950C)24,8001WN6h11.89
HD 97950 (WR 43)25,0001WR9.03It is the central core of a super star cluster within the NGC 3603 H II region (similar to R136 within the Tarantula Nebula).
Arches-F1 (WR 102ad)25,0001WN8-9h
Arches-F6 (WR 102ah)25,0001WN8-9h
Arches-F9 (WR 102ae)25,0001WN8-9h
WR 42e (2MASS J11144550-115001)25,0001O3If*/WN614.53
G0.059-0.068 26,0001B0-1Ia+/WNLh
G0.238-0.071 26,0001WN11hPresent in the Galactic Center region of Milky Way.
WR 102ka (Peony Star)26,0001Ofpe/WN9
WR 102c 26,0001WN611.6
WR 102ea 26,0001WN9h8.8
GCIRS 13E (WR 101f)26,0001WRLocated near Galactic Center.
GCIRS 16SW 26,0001Ofpe/WN9Located near Galactic Center.
WR 101-2 (CXOGC J174516.1-284909)26,0921Ofpe/WN9
WR 31a (Hen 3-519)28,0001WN11h10.85
WR 102e 28,0001WR
WR 150 28,473+1,700
−1,380
1WC513.47
HD 826 30,0001WC8Center Star of NGC 40 Nebula.
WR 102b 31,0001WR
Mercer 30-1 A (WR 46-3 A)40,0001WR
Mercer 30-7 A40,0001WR

Magellanic Clouds

The Large Magellanic Cloud (LMC) is around 163 kly distant and the Small Magellanic Cloud (SMC) is around 204 kly distant

Host galaxyStar systemMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
LMC LMC195-1 160,0001WO215.15
LMC LH 41-1042 160,0001WO413.95
LMC R145 (HD 269928)163,0002WN6h + O3.5If*/WN712.04
LMC HD 38282 (BAT99-118/Brey 89)163,0002WN5-6h + WN6-7h11.11
LMC BAT99-7 163,0001WN4b13.81
LMC BAT99-123 (Brey 93)163,0001WO315.204
LMC Melnick 34 (BAT99-116)163,0002WN5h + WN5h13.09
LMC R136a1 (RMC 136a1)163,0001WN5h12.23
LMC R136a2 (RMC 136a2)163,0001WN5h12.34
LMC R136a3 163,0001WN5h12.97
LMC R136c 163,0001WN5h12.86
LMC R71 (HD 269006)164,0001WR8.7 - 9.9 - 11.2
LMC VFTS 457 164,0001O3.5If*/WN7
LMC VFTS 482 164,0001O3If*/WN6-A
LMC VFTS 545 164,0001O2If*/WN5
LMC VFTS 682 164,0001WN5h16.08
LMC VFTS 1022 164,0001O3.5If*/WN7
LMC R134 164,0001WR
LMC R146 164,0001WN4
LMC BAT99-98 165,0001WN613.38
LMC R99 165,0001Ofpe/WN1011.46
SMC SMC AB7 197,0002WN413.016
SMC SMC AB8 197,0002WO412.83
SMC HD 5980 200,0001WN48.8 - 11.9

Andromeda Galaxy and Triangulum Galaxy

The Andromeda Galaxy (M31) is 2.5 Mly distant and the Triangulum Galaxy is around 3.2 Mly distant

Host galaxyStar systemMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
Triangulum [BMS2003] 867 2,700,0002O4Iab+O4Ia
Triangulum Romano's Star 2,700,0002WN8h–WN11h16.5–18.8

Other Galaxies

Host GalaxyStar systemMedian distance (ly)Stars in system Spectral type Apparent magnitude (V)Comments and references
NGC 6822 NGC 6822-WR 12 (LGGS J194513.50-144512.9)1,540,0001WN418.96

See also

Related Research Articles

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<span class="mw-page-title-main">R Sagittae</span> Star in the constellation Sagitta

R Sagittae is an RV Tauri variable star in the constellation Sagitta that varies from magnitude 8.0 to 10.5 in 70.77 days. It is a post-AGB low mass yellow supergiant that varies between spectral types G0Ib and G8Ib as it pulsates. Its variable star designation of "R" indicates that it was the first star discovered to be variable in the constellation. It was discovered in 1859 by Joseph Baxendell, though classified as a semi regular variable until RV Tauri variables were identified as a distinct class in 1905.

<span class="mw-page-title-main">NGC 121</span> Globular cluster in the constellation Tucana

NGC 121 is a globular cluster of stars in the southern constellation of Tucana. It is the oldest globular cluster in the Small Magellanic Cloud (SMC), which is a dwarf satellite galaxy of the Milky Way. This cluster was first discovered by English astronomer John Herschel on September 20, 1835. The compiler of the New General Catalogue, Danish astronomer John Louis Emil Dreyer, described this object as "pretty bright, pretty small, little extended, very gradually brighter middle". The cluster is located at a distance of around 200,000 light-years (60 kpc) from the Sun.

<span class="mw-page-title-main">HV 11423</span> Star in the Small Magellanic Cloud in the constellation Tucana

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References

  1. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics . 616. A1. arXiv: 1804.09365 . Bibcode: 2018A&A...616A...1G . doi: 10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
  2. Barry, Don C. (January 1970), "Spectral Classification of a and F Stars", Astrophysical Journal Supplement, 19: 281, Bibcode:1970ApJS...19..281B, doi:10.1086/190209.
  3. Frost, E. B. (December 1924), "Fourteen spectroscopic binaries", Astrophysical Journal, 60: 319–320, Bibcode:1924ApJ....60..319F, doi:10.1086/142868.