The Mass-Luminosity Relation from End to End

Details The Mass-Luminosity Relation from End to End The Mass-Luminosity Relation from End to End

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..159h&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

13

Scientific paper

We provide a review of the progress made in mapping out the stellar mass-luminosity relation over more than two decades. The 2004 version of the mass-luminosity relation spans stellar masses spanning the range of 0.07 to 33 M&sun;. Special emphasis is given to the red dwarfs, which comprise roughly half of the Galaxy's stellar mass even though they have the lowest stellar masses.

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