NGC 2903 and NGC 4569: possible X-ray emission from the halos of two nuclear starburst galaxies.

Details NGC 2903 and NGC 4569: possible X-ray emission from the halos of two nuclear starburst galaxies. NGC 2903 and NGC 4569: possible X-ray emission from the halos of two nuclear starburst galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..459j&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 459 - 460

Astronomy and Astrophysics

Astrophysics

2

Starburst Galaxies: X Rays, Starburst Galaxies: Spiral Galaxies, Starburst Galaxies: Nearby Galaxies

Scientific paper

The authors present the results of an X-ray investigation of two nearby spiral galaxies, NGC 2903 and NGC 4569. Observations with the ROSAT PSPC detector show extended X-ray emission from the nuclei and from the disks of both galaxies. The total amount of soft X-ray emission can be solely explained with ongoing starburst activity. A part of the X-ray emission originate from a region outside the disk and could be associated with hot gas from the halo of these galaxies.

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