On Determining the Sources of Hot Gas in the Ha

Details On Determining the Sources of Hot Gas in the Ha On Determining the Sources of Hot Gas in the Ha

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9..259s&link_type=abstract

"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,

Astronomy and Astrophysics

Astrophysics

Scientific paper

The hot gas above the Galactic Disk provides an interesting and important puzzle. Could this gas have been advected from hot bubbles formed in the disk, dropped upon the Galaxy from above, or heated in situ? Each of these possibilities has important ramifications for the functioning of the Galaxy, magnifying the need for better tests. In this paper, several theoretical models for hot gas in the halo, their ionization history, and spectral appearances will be discussed, along with a scheme for using the emerging set of soft X-ray and far ultraviolet observatories to distinguish between classes of models.

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