Limits to pressure in stars and velocity dispersions in stellar systems.

Details Limits to pressure in stars and velocity dispersions in stellar systems. Limits to pressure in stars and velocity dispersions in stellar systems.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...302..924m&link_type=abstract

Astronomy and Astrophysics, v.302, p.924

Astronomy and Astrophysics

Astrophysics

2

Stars: Interiors, Stellar Dynamics, Galaxies: Kinematics And Dynamics, Globular Clusters: General

Scientific paper

New, rigorous, upper and lower limits to pressure in outer layers of spherically symmetric mass distributions in hydrostatic equilibrium are presented. Upper and lower limits to general integrals of stellar variables are obtained and illustrated. The pressure inequalities translate into rigorous, upper and lower limits for velocity dispersion in isotropic, spherically symmetric stellar systems. They set lower limits to gravitational masses of galaxies in terms of the X-ray temperatures of the gas they contain.

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