Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-04-15
Astrophys.J.628:973-985,2005
Astronomy and Astrophysics
Astrophysics
32 pages, 16 figures; Accepted by the Astrophysical Journal
Scientific paper
10.1086/430901
We use moderate-resolution optical spectrophotometry and the new MARCS stellar atmosphere models to determine the effective temperatures of 74 Galactic red supergiants. From these we find a new effective temperature scale that is significantly warmer than those in the literature. We show that this temperature scale, along with the newly derived bolometric corrections, gives much better agreement between our red supergiants and stellar evolutionary tracks. This agreement provides an independent verification of our new temperature scale. The combination of effective temperature and bolometric luminosities allows us to calculate stellar radii; the coolest and most luminous stars have radii of roughly 1500 solar radii (7 AU), in excellent accordance with the largest stellar radii predicted from current evolutionary theory. We find that similar results are obtained for the effective temperatures and bolometric luminosities using only the de-reddened V-K colors, providing a powerful demonstration of the self-consistency of the MARCS models.
Josselin Eric
Levesque Emily M.
Maeder Andre
Massey Philip
Meynet Georges
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