The interaction of high-velocity-clouds with the galactic disk

Details The interaction of high-velocity-clouds with the galactic disk The interaction of high-velocity-clouds with the galactic disk

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995adspr..16q.119k&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 16, no. 3, p. 119-122

Astronomy and Astrophysics

Astronomy

4

Chemical Composition, Galactic Halos, Molecular Clouds, Plasma Temperature, Rosat Mission, X Ray Astronomy, Brightness Temperature, Emission Spectra, Energy Spectra, Energy Transfer, Magnetic Fields

Scientific paper

Recently evidence was presented for enhanced soft X-ray emission associated with a high-velocity-cloud (HVC). We now present additional observational results with indicate that the X-ray emission is indeed produced by the impact of the HVC onto the galactic disk. Moreover, we present first estimations about the energy budget of the interaction area.

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