Stellar mass-luminosity and mass-radius relations

Details Stellar mass-luminosity and mass-radius relations Stellar mass-luminosity and mass-radius relations

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.181..313d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 181, no. 2, July 1991, p. 313-322.

Astronomy and Astrophysics

Astrophysics

51

Binary Stars, Main Sequence Stars, Mass To Light Ratios, Radii, Stellar Luminosity, Stellar Mass, Parameterization, Regression Analysis, Stellar Models

Scientific paper

The mass-luminosity and mass-radius relations (MLR and MRR) for main-sequence stars are investigated using recent binary star data together with new theoretical estimates. The slopes of the relations are found to change at certain critical values, e.g., at about 0.5 solar mass for MLR and at about 1.7 solar mass for MRR. The results obtained demonstrate the relative tightness, importance, and usefulness of the MLR and MRR.

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