Filling the Yellow Void: A Census of F and G Supergiants in M31

Details Filling the Yellow Void: A Census of F and G Supergiants in M31 Filling the Yellow Void: A Census of F and G Supergiants in M31

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..425...51d&link_type=abstract

Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series Vol. 425, Proceedings of a Workshop held at the Cali

Astronomy and Astrophysics

Astronomy

Scientific paper

The yellow supergiant population of a galaxy can act as a very stringent test of the current evolutionary models. However, this portion of the color magnitude diagram is dominated by foreground contamination, indicating a new means of supergiant distinction is necessary. We now present the results from a census of F- and G-type supergiants in M31 based on radial velocity, and the subsequent testing of the current Geneva evolutionary tracks.

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