The gaseous Halo of the Virgo Cluster Galaxy 45

Details The gaseous Halo of the Virgo Cluster Galaxy 45 The gaseous Halo of the Virgo Cluster Galaxy 45

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..467h&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 467-470 (2003).

Astronomy and Astrophysics

Astrophysics

1

Galaxies: Active, Galaxies: Starburst, Galaxies: Individual: Ngc 456, Galaxies: Halos

Scientific paper

Observations of the Virgo Cluster galaxy NGC 4569 in soft X-rays and in Hα reveal both an asymmetrically distributed hot gaseous halo and a giant filament of diffuse emission, respectively, extending from the same side of the disk, the latter one to at least 8.8 kpc. A deep longslit spectrum along the filament shows velocities systematically different from the systemic velocity of NGC 4569. With the inclination of the disk one can determine the Hα spur as a giant outflow in NGC 4569.

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