Measuring mass-to-light ratios of spherical stellar systems by core fitting

Details Measuring mass-to-light ratios of spherical stellar systems by core fitting Measuring mass-to-light ratios of spherical stellar systems by core fitting

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....92...72r&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 92, July 1986, p. 72-74.

Physics

107

Mass To Light Ratios, Star Clusters, Stellar Physics, Stellar Systems, Polytropic Processes, Spheres, Stellar Cores, Stellar Models

Scientific paper

The authors discuss the determination of mass-to-light ratios of
spherical stellar systems by core fitting (King's method). They justify
the core-fitting formula and state the conditions for its validity.

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