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- Q1401599 subject Q7009483.
- Q1401599 subject Q7282805.
- Q1401599 subject Q8432416.
- Q1401599 subject Q8606655.
- Q1401599 abstract "VHK 83 (Var 83 in the VHK survey) 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" 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. 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.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.".
- Q1401599 wikiPageWikiLink Q10565.
- Q1401599 wikiPageWikiLink Q105902.
- Q1401599 wikiPageWikiLink Q1141760.
- Q1401599 wikiPageWikiLink Q13724.
- Q1401599 wikiPageWikiLink Q1454942.
- Q1401599 wikiPageWikiLink Q2703.
- Q1401599 wikiPageWikiLink Q7009483.
- Q1401599 wikiPageWikiLink Q7282805.
- Q1401599 wikiPageWikiLink Q742741.
- Q1401599 wikiPageWikiLink Q8432416.
- Q1401599 wikiPageWikiLink Q8606655.
- Q1401599 type Place.
- Q1401599 type CelestialBody.
- Q1401599 type Location.
- Q1401599 type Place.
- Q1401599 type Star.
- Q1401599 type Thing.
- Q1401599 comment "VHK 83 (Var 83 in the VHK survey) 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" 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.".
- Q1401599 label "Var 83".
- Q1401599 name "VHK 83".