Chandra Detection of a Hot Gaseous Corona Around the Edge-on Galaxy NGC 4631

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3 pages, 8 figures. To appear in ApJ Letters. Full resolution version available at http://xray.astro.umass.edu/n4631.ps.gz

Scientific paper

10.1086/323179

We present a Chandra X-ray observation that shows, unambiguously for the first time, the presence of a giant diffuse X-ray-emitting corona around the edge-on disk galaxy NGC 4631. This corona, with a characteristic thermal temperature of 2-7\times10^6 K, extends as far as 8 kpc away from the galactic plane. The X-ray morphology resembles the radio halo of the galaxy, indicating a close connection between outflows of hot gas, cosmic rays, and magnetic field from the galactic disk. Enhanced diffuse X-ray emission is apparently enclosed by numerous H\alpha-emitting loops blistered out from the central disk of the galaxy, as is evident in a comparison with our deep Hubble Space Telescope imaging.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Chandra Detection of a Hot Gaseous Corona Around the Edge-on Galaxy NGC 4631 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Chandra Detection of a Hot Gaseous Corona Around the Edge-on Galaxy NGC 4631, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chandra Detection of a Hot Gaseous Corona Around the Edge-on Galaxy NGC 4631 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-555086

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.