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This is a list of luminous blue variable stars in order of their distance from Earth.[1][2][3]
Star system | Nebula | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|---|
P Cygni (34 Cygni) | 5251±180 | 1 | B1-2 Ia-0ep | 4.82 | The closest luminous blue variable star to Earth | |
V4029 Sagittarii (HD 168607) | 6,000 | 1 | B9Ia+ | 8.12 to 8.29 | [4][5] near the Omega Nebula | |
V905 Scorpii (HD 160529) | 6,100 | 1 | LBV | 6.66 | [4][5] | |
Eta Carinae (Eta Argus) | 7,500 | 2 | O + B | −1.0 to ~7.6 | part of Trumpler 16 in the Carina Nebula | |
MWC 930 (V446 Scuti) | 11,400 | 1 | B5/9Iaeq | 11.51 | [4] | |
WRAY 16-137 | 12,400 | 1 | LBV | 15.5 | [6][5] | |
W1-243 | 15,000 | 1 | LBV | 15.81 | [4] in Westerlund 1 | |
HR Carinae | 16,000 | 2 | LBV+RSG | 8.42 | [4][5] | |
V481 Scuti (LBV G24.73+0.69) | 17,000 | 1 | LBV_B[e]: | [4] | ||
AG Carinae | 17,000 ± 1,000 | 1 | B | 6.96 | ||
EM* VRMF 55 (MN44) | 18,000 or 35,000 | 1 | LBV | 15 | [6][7] | |
[GKF2010] MN48 | 20,000 | 1 | 15.83 | [4][5] | ||
GCIRS 34W (WR 101db) | 25,000 | 1 | Ofpe/WN9 | [6][8] in the galactic center | ||
Pistol Star (V4647 Sgr) | 25,114 | 1 | B | >28 | part of the Quintuplet cluster | |
LBV G0.120-0.048 (V4998 Sgr) | 26,000 | 1 | WN5b | [6] near the Quintuplet cluster | ||
FMM 362 (V4650 Sgr) | 26,000 | 1 | LBV | [6] near the Quintuplet cluster | ||
AFGL 2298 (V1672 Aql) | 30,000 | 1 | B8I | [6] | ||
V432 Carinae (Wray 15-751) | 33,000 | 1 | LBV | 10.20 | Also known as AT 2019ooa[4][5] | |
[GKM2012] WS1 | 39,000 | 1 | LBV | 15.31 | [4][5] | |
[GKF2010] MN58 | 1 | [6] | ||||
Star system | Nebula | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|---|
HD 148937 | 3,870 | 1 | O6f?p | 6.71 | [6] central star of NGC 6164 | |
MWC 349A (V1478 Cygni) | 4,560 | 2–3 | B0-1.5 I + B0 III | 13.15 | [6] maybe ejected from Cygnus OB2 | |
HD 326823 | 4,700 | 1 | WNpec | 9.03 | [4][5] | |
HD 168625 | 5,000 | 1 | B6Ia+ | 8.30–8.41 | [4][5] near the Omega Nebula | |
Cygnus OB2-12 | 5,500 | 1 | B3–4 Ia+ | 11.702 | [4][5] in Cygnus OB2 | |
AS 314 | 5,600 | 1 | B9Ia | 9.85 | [6] | |
Zeta1 Scorpii | 5,600 | 1 | B1.5 Iae | 4.705 | [4][5] | |
G79.29+0.46 | 5,700 | 1 | B:I[e] | 15.1 | [4][5] in Cygnus X | |
WRAY 16-232 | 6,850 | 1 | Be | 12.5 | [6][5] | |
HD 80077 | 8,700 | 1 | B2.5Ia+ | 9.00 | [4][5] | |
HD 316285 | 10,800 | 1 | B0Ieq | 9.60 | [4][5] | |
MWC 314 (V1429 Aquilae) | 15,000 | 3 | B3Ibe | 9.79 - 10.1 | [4][5] | |
[SBW2007] 1 | 18,500 | 1 | B1Iab | 12.7 | [4][5] | |
Sher 25 | 21,000 | 1 | cLBV | 12.23 | [4][5] in NGC 3603 | |
W51 LS1 (V1936 Aquilae) | 22,000 | 1 | O4I | 15.1 | [4][5] | |
WRAY 17-96 | 22,000 | 1 | cLBV | ~13.0 | [4][5] | |
[B61] 2 | 22,000 | 1 | LBV_B[e]: | 15.00 | [6][5] | |
WR 102ka | 26,000 | 1 | WN10 | [6] near the galactic center | ||
GCIRS 16SW | 27,000 | 1 | Ofpe/WN9 | [6] in the galactic center | ||
LBV 1806−20 | 28,000 | 1 | cLBV | [6] part of the 1806−20 cluster | ||
Hen 3-519 | 28,000 | 1 | WN11h | 10.85 | [4][5] | |
MSX6C G026.4700+00.0207 | 30,000 | 1 | LBV_B | [6][9] |
The Large Magellanic Cloud (LMC) is around 163 kly distant and the Small Magellanic Cloud (SMC) is around 204 kly distant
Host galaxy | Star system | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
LMC | S Doradus | 1 | B8/9eq – F0/5:Iae | 8.6 – 11.5 | |
LMC | HD 269858 (R127) | 1 | B | 10.15 | |
LMC | HD 269006 (R71) | 1 | LBV | 10.55 | [6] |
LMC | HD 269216 (SK −69 75) | 1 | OBe | 11.123 | [6] |
LMC | HD 269582 (SK −69 142a) | 1 | WN10h | 11.093 | [6] |
LMC | HD 269662 (R110) | 1 | A0Ia | 10.28 | [6] |
LMC | HD 269700 (R116) | 1 | B1.5Iaeq | 10.54 | [6] |
LMC | R143 (CPD-69 463) | 1 | F7Ia | 12.014 | [6] |
SMC | HD 5980 (R14) | 3 | WN4+O7I: | 11.31 | [6] |
SMC | HD 6884 (R40) | 1 | B9Ia0ek | 10.2 | [6] |
The Andromeda Galaxy (M31) is 2.5 Mly distant and the Triangulum Galaxy is around 3.2 Mly distant
Host galaxy | Star system | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|
Andromeda | LGGS J004051.59+403303.0 | 1 | LBV | 16.989 | [6] |
Andromeda | AE Andromedae (HV 4476) | 1 | LBV | 17.0–17.9 | [6] |
Andromeda | AF Andromedae (HV 4013) | 1 | LBV | 17.325 | [6] |
Andromeda | Var 15 ([WB92a] 370) | 1 | LBV | 18.450 | [6] |
Andromeda | Var A-1 | 1 | LBV | 17.143 | [6] |
Andromeda | UCAC4 660-003111 | 1 | LBV | 16.39 | [6] |
Triangulum | Var C | 1 | LBV | 16.429 | [6] |
Triangulum | Var B | 1 | LBV | 16.208 | [6] |
Triangulum | Var 83 | 1 | LBV | 15.4–16.6 | [6] |
Triangulum | Var 2 (Y Trianguli) | 1 | Ofpe/WN9 | 18.22 | [6] |
Triangulum | Romano’s Star (M33 V0532) | 1 | Ofpe/WN9 | 16.5–18.8 | [6] |
Host Galaxy | Star system | Median distance (ly) | Stars in system | Spectral type | Apparent magnitude (V) | Comments and references |
---|---|---|---|---|---|---|
NGC 3109 | AT 2018akx | 4,350,000 | 1 | LBV | 17.5 - 19.28 | [10] |
NGC 2403 | AT 2016ccd | 9,650,000 | 1 | LBV | 18.0 - 19.95 | Also known as SNhunt225.[11][12] |
NGC 4214 | SN 2010U | 9,700,000 | 1 | LBV | 16 | [13] |
NGC 2363 | NGC 2363-V1 | 10,800,000 | 1 | LBV | 17.88 | One of the most luminous stars known. |
NGC 45 | AT 2018htr | 21,700,000 | 1 | LBV | 17.469 | [14] |
NGC 2537 | AT 2017be | 27,900,000 | 1 | LBV | 18.349 - 18.5 | Distance from NED using redshift of host galaxy.[15] |
NGC 4559 | AT 2016blu | 29,000,000 | 1 | LBV | 15.9 – 19 | Repeated outbursts have been observed since January 2012.[16][17] |
NGC 7286 | AT 2019mil | 32,400,000 | 1 | LBV | 19 | Distance from NED using redshift of host galaxy.[18] |
UGC 5829 | AT 2021blu | 43,500,000 | 1 | LBV | 18.17 - 21.62 | Distance from NED using redshift of host galaxy.[19] |
NGC 4656 | Variable in NGC 4656 | 43,700,000 | 1 | LBV | 18 | Distance from NED using redshift of host galaxy.[20] |
NGC 4389 | AT 2022fnm | 44,700,000 | 1 | LBV | 18.495 - 17.855 | Distance from NED using redshift of host galaxy.[21] |
ESO 249- G 015 | AT 2020agp | 47,500,000 | 1 | LBV | 18.463 | Distance from NED using redshift of host galaxy.[22] |
NGC 908 | AT 2021ablz | 56,000,000 | 1 | LBV | 20.58 | [23] |
UGC 5979 | SN 2007sv | 58,270,000 | 1 | LBV | 17.4 | Distance from NED using redshift of host galaxy.[24][25] |
IC 5267A | AT 2019oet | 60,000,000 | 1 | LBV | 18.335 | Distance from NED using redshift of host galaxy.[26] |
NGC 2748 | PSN J09132750+7627410 | 61,300,000 | 1 | LBV | 18.3 | [27] |
NGC 3423 | AT 2019ahd | 65,600,000 | 1 | LBV | 17.83 - 18.73 | Distance from NED using redshift of host galaxy.[28] |
NGC 1385 | AT 2020pju | 66,400,000 | 1 | LBV | 17.3 - 19.73 | [29] |
NGC 718 | AT 2019udc | 69,800,000 | 1 | LBV | 17.53 - 19.09 | Distance from NED using redshift of host galaxy.[30] |
NGC 5334 | SN 2003gm | 80,196,000 | 1 | LBV | 17.0 | Distance from NED using redshift of host galaxy.[31] |
SDSS J094838.45+332529.1 | AT 2020jev | 80,200,000 | 1 | LBV | 18.74 - 20.33 | Distance from NED using redshift of host galaxy.[32] |
NGC 6509 | PSN J17592296+0617267 | 95,300,000 | 1 | LBV | 18.5 | [33] |
NGC 4045 | AT 2019wbg | 111,500,000 | 1 | LBV | 17.7 -19.39 | Repeated outbursts observed since discovery. Distance from NED using redshift of host galaxy.[34] |
NGC 4532 | AT 2017des | 112,800,000 | 1 | LBV | 18.817 - 19.85 | Distance from NED using redshift of host galaxy.[35][36] |
ESO 602- G 015 | AT 2022rmk | 113,200,000 | 1 | LBV | 19.472 - 20.04 | Distance from NED using redshift of host galaxy.[37] |
UGC 9113 | AT 2017dau | 162,100,000 | 1 | LBV | 19.32 - 21.32 | Distance from NED using redshift of host galaxy.[38] |
MCG +07-07-070 | AT 2018kle | 180,200,000 | 1 | LBV | 18.797 - 18.91 | Distance from NED using redshift of host galaxy.[39] |
UGC 449 | AT 2022oku | 239,100,000 | 1 | LBV | 18.781 - 19.49 | Distance from NED using redshift of host galaxy.[40] |
WISEA J010803.49+010843.7 | AT 2020zmn | 262,600,000 | 1 | LBV | 20.31 - 20.85 | Distance from NED using redshift of host galaxy.[41] |
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