Galactic Winds and the X-ray Luminous Bulges of Spiral Galaxies

Details Galactic Winds and the X-ray Luminous Bulges of Spiral Galaxies Galactic Winds and the X-ray Luminous Bulges of Spiral Galaxies

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543204w&link_type=abstract

American Astronomical Society, AAS Meeting #215, #432.04; Bulletin of the American Astronomical Society, Vol. 42, p.367

Astronomy and Astrophysics

Astronomy

Scientific paper

Galactic winds are typically associated with galaxies that host AGN or are undergoing vigorous star formation. The discovery of the overpressurized hot gas in the bulge of NGC 3631 inspired the investigation of several more normal, quiescent spiral galaxies_all with an X-ray luminous bulge. The sample was studied with the WIYN 3.5m. We present the results of an integral field unit study of the kinematics of ionized and neutral gas in the bulges of spiral galaxies and discuss the frequency of galactic winds amongst "normal” early-type spirals.

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