Gone With The Galactic Wind: Observation and Theory

Details Gone With The Galactic Wind: Observation and Theory Gone With The Galactic Wind: Observation and Theory

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.6025l&link_type=abstract

American Astronomical Society Meeting 205, #60.25; Bulletin of the American Astronomical Society, Vol. 36, p.1446

Astronomy and Astrophysics

Astronomy

Scientific paper

The study of X-ray emitting diffuse gas in galactic halos is of importance in understanding the formation and evolution of galaxies. A spherical steady galactic wind model is developed and confronted with the Chandra observation of the bulge-dominated edge-on Sa galaxy M104. We derive super-solar abundances for Fe-like elements from spectral fit, which is consistent with ISM enrichment predominated by Type Ia supernovae in the galactic bulge.

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