The influence of overshooting and stellar wind mass loss in the mass-luminosity relation

Details The influence of overshooting and stellar wind mass loss in the mass-luminosity relation The influence of overshooting and stellar wind mass loss in the mass-luminosity relation

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..155f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 1, Dec. 1991, p. 155-158. Research supported by Junta Nacional de Inv

Mathematics

Logic

Mass To Light Ratios, Stellar Mass Ejection, Stellar Winds, Main Sequence Stars, Stellar Evolution, Stellar Luminosity, Stars: Main-Sequence, Stars: Evolution Of, Stars: Mass Loss, Mass-Luminosity Relation

Scientific paper

The effect of overshooting and stellar wind mass loss on the position of stellar models in the mass-luminosity diagram is examined. The average main sequence is well represented log L/Lsun = 2.47 log M/Msun + 1.52. The influence of variations in the amount of overshooting or the mass loss rate is rather small, and the exponent in the ML-relation varies around 2.5. The theoretical results are compared to corresponding relations derived from observations. The importance of the limiting mass values on the result is discussed.

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