Article snapshot taken from Wikipedia with creative commons attribution-sharealike license.
Give it a read and then ask your questions in the chat.
We can research this topic together.
Assigned spectral classes for 12 Aurigae vary greatly from B2 to B5 and the luminosity class from V (main sequence) to Ia (luminous supergiant). Its spectrum shows prominent emission lines, but the spectrum is complicated by the appearance of sharp shell components to some of the spectral lines. The colour of the star as shown by the B-V and U-B colour indices is not consistent with an early B spectral class, leading to many estimates of its effective temperature that are much lower than expected for a B-class star. The expected temperature for a B5 spectral type would be 15,400 K, but most sources assign a temperature of around 8,000 K. Other properties also vary between different sources, for example the bolometric luminosity derived from the distance and temperature is 25 L☉, while it is 635 L☉ when derived by fitting the spectral energy distribution. A calculation of the stellar properties assuming the maximum possible interstellar extinction in the direction of 12 Aurigae results in a temperature of 14,336 K and a luminosity of 8,092 L☉, although it is strongly noted that the likely extinction is much lower.
Category