The X-ray emission of galaxies.

Details The X-ray emission of galaxies. The X-ray emission of galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..347f&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 347 - 356

Astronomy and Astrophysics

Astrophysics

11

Galaxies: X Rays

Scientific paper

Galaxies have been observed and studied in X-rays for the past ≡15 yr. Not surprisingly, they are complex X-ray sources, consisting of populations of bright individual sources (accretion binaries, SNR, SN), increasingly complex gaseous components, and sometimes active nuclei, not to mention the baseline stellar coronal emission. Through X-ray observations there is direct evidence of the chemical and dynamical interaction between galaxies and the surrounding medium; one can observe directly the most massive sources in these galaxies (either super-Eddington accretion binaries or AGN); one can probe into the structure and evolution of E and S0 galaxies.

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