Title

The physical properties of red supergiants

Document Type

Conference Proceeding

Publication Date

12-1-2008

Abstract

The "observed" location of red supergiants in the HRD has been at variance with the evolutionary tracks for many years, but the new generation of MARCS stellar atmosphere models has led to improved determinations of their physical properties, and much better agreement with stellar evolutionary theory. We briefly summarize our findings. © 2008: Instituto de Astronomía.

Publication Source (Journal or Book title)

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias

First Page

29

Last Page

31

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