Multiple Stars and Stellar Evolution

Details Multiple Stars and Stellar Evolution Multiple Stars and Stellar Evolution

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1314..128k&link_type=abstract

INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink's 65th Birthday. AIP Conference Proceedings, Volume 1314, p

Physics

Stellar Evolution, Multiple Stars, Brightness, Stellar Winds, White Dwarfs, Black Holes, Multiple Stars, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Mass Loss And Stellar Winds, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

We discuss the incidence of multiplity, particularly among the bright and therefore relatively thoroughly examined stars, and note certain types of (a) binary stars that might be expected to merge, and (b) single stars with characteristics that suggest they may be former binaries that merged. Some Be stars and rapidly rotating red giants seem like possible merger products; and perhaps even some magnetic peculiar stars that are rapidly rotating.

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