Var 83
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Triangulum |
| Right ascension | 01h 33m 50.02s |
| Declination | +30° 39′ 36.7″ |
| Apparent magnitude (V) | 15.4-16.6[1] |
| Characteristics | |
| Spectral type | LBV |
| U−B color index | -0.9v[1] |
| B−V color index | 0.1v[1] |
| Variable type | LBV |
| Astrometry | |
| Proper motion (μ) | RA: 11.54 mas/yr Dec.: -2.75 mas/yr |
| Distance | ~3,000,000 ly (~900,000 pc) |
| Absolute magnitude (MV) | −8.4- −9.5[1] |
| Details | |
| Mass | 60-85[2] M☉ |
| Radius | 50-80[1]-150[3] R☉ |
| Luminosity | 2,100,000-4,500,000[3] L☉ |
| Temperature | 18,000-37,000[3][1] K |
| Other designations | |
Var 83, VHK 83, 2MASS J01341090+3034373 | |
| Database references | |
| SIMBAD | data |
VHK 83 (Var 83 in the VHK survey[4]) is a luminous blue variable (LBV) in the constellation Triangulum, in the Triangulum Galaxy. With its bolometric luminosity of at least 2,240,000 times that of the Sun (4,500,000 in some estimates), it was described as "the brightest nonstable star in M33"[4] and is one of the most luminous stars known.
The brightness varies slowly and unpredictably over a 1-2 magnitude visual range and can remain approximately constant for many years. These variations, combined with the high luminosity and temperature of the star, caused it to be grouped with the Hubble-Sandage variables even before the term "Luminous Blue Variable" was more than a simple description.[5] Despite widespread agreement that it is an LBV it has yet to be observed in outburst, although the temperature has been observed to change in tandem with the brightness variations.[1]
Temperature estimates for the star range from around 18,000K to well over 30,000K. The hotter temperatures found from fitting the spectral energy distribution (SED) are consistent with the calculated luminosity of an LBV in the quiescent stage, but the spectrum is that of a cooler star.[3]
References
- ^ a b c d e f g Attention: This template ({{cite doi}}) is deprecated. To cite the publication identified by doi:10.1086/161774, please use {{cite journal}} (if it was published in a bona fide academic journal, otherwise {{cite report}} with
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- ^ a b c d Attention: This template ({{cite doi}}) is deprecated. To cite the publication identified by doi:10.1111/j.1745-3933.2009.00654.x, please use {{cite journal}} (if it was published in a bona fide academic journal, otherwise {{cite report}} with
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|doi=10.1086/190344instead. - ^ Attention: This template ({{cite doi}}) is deprecated. To cite the publication identified by doi:10.1086/155797, please use {{cite journal}} (if it was published in a bona fide academic journal, otherwise {{cite report}} with
|doi=10.1086/155797instead.
Further reading
- VHK Survey: Astrophysical Journal Supplement Series, "A Survey of Bright Variable Stars in M33"; van den Bergh, S.; Herbst, E.; Kowal, C. T.; (Supplement no. 287), vol. 29, July 1975, p. 303-313. Bibcode:1975ApJS...29..303V ; doi:10.1086/190344 ;
- Astronomical Journal, "LBV-Type Stars in M33", Corral, L. J.; v.112, p. 1450, 10/1996; Bibcode:1996AJ....112.1450C ; doi:10.1086/118113 ;
