Elliptical galaxies - Optical and X-ray properties and predictions of the hot model of galaxy formation

Details Elliptical galaxies - Optical and X-ray properties and predictions of the hot model of galaxy formation Elliptical galaxies - Optical and X-ray properties and predictions of the hot model of galaxy formation

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..216s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, March 1989, p. 216-222. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Elliptical Galaxies, Galactic Evolution, Optical Properties, Stellar Models, X Ray Astronomy, Brightness Distribution, Prediction Analysis Techniques, Stellar Coronas, Stellar Luminosity

Scientific paper

It is shown that the hot model can be used to explain the dimensions of E galaxies. This model can also be used to predict the existence of a relationship between: (1) the temperature of X-ray coronae and surface brightness, and (2) the luminosity, the dispersion of stellar velocities, and surface brightness. The latter relation is consistent with the Faber-Jackson relation.

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