Giant Binary Stars and the Mass-Luminosity Law

Details Giant Binary Stars and the Mass-Luminosity Law Giant Binary Stars and the Mass-Luminosity Law

Nov 1948

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1948natur.162..815h&link_type=abstract

Nature, Volume 162, Issue 4125, pp. 815-816 (1948).

Physics

1

Scientific paper

IT is well known that spectroscopic parallaxes are an index of stellar surface gravity, which in turn is functionally related to the mass and luminosity of a star. If, therefore, there exists a class of stars in which this functional relation differs from that found for the majority of stars, we should expect a lack of agreement of the mean trigonometric, dynamic and spectroscopic parallaxes of these stars.

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