The physical association of high-velocity clouds with soft X-ray emission.

Details The physical association of high-velocity clouds with soft X-ray emission. The physical association of high-velocity clouds with soft X-ray emission.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..327k&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 327 - 328

Astronomy and Astrophysics

Astrophysics

High-Velocity Clouds: X Rays

Scientific paper

The authors review the recent arguments that high-velocity clouds (HVCs) are physically associated with soft X-ray emission. The analysis of ROSAT PSPC and H I 21 cm line data reveal several independent indications that soft X-ray emission originates close to the HVC rims. This is the first firm large scale detection of HVCs in emission since their discovery in the H I 21 cm line radiation by Muller et al. in 1963.

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