X-rays and dynamics

Details X-rays and dynamics X-rays and dynamics

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15...91p&link_type=abstract

Highlights of Astronomy, Volume 15, p. 91-91

Astronomy and Astrophysics

Astronomy

Galaxies: Elliptical And Lenticular, Cd, Galaxies: Fundamental Parameters, Galaxies: Halos, Galaxies: Ism, Galaxies: Kinematics And Dynamics, Galaxies: Structure

Scientific paper

The hot X-ray emitting interstellar medium of early type galaxies can be used in principle as a total mass tracer and a tool to determine the stellar orbital anisotropy, based on the hypothesis of hydrostatic equilibrium for it. Here the effects that deviations from equilibrium have on both estimates are shown, and a comparison is made with cases for which accurate optical and X-ray information are available.

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