X-ray emission from UGC 6697 in A 1367

Details X-ray emission from UGC 6697 in A 1367 X-ray emission from UGC 6697 in A 1367

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..293f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 2, April 1990, p. 293-297.

Astronomy and Astrophysics

Astronomy

4

Galactic Clusters, Irregular Galaxies, Stellar Luminosity, X Ray Sources, Peculiar Stars, Radio Emission, Sky Surveys (Astronomy)

Scientific paper

Reanalysis of two overlapping HRI observations of the cluster of
galaxies A 1367 leads to the detection of an X-ray source identified
with the peculiar/irregular galaxy Zw 97-087 (UGC 6697). The observed
luminosity can be contributed by discrete X-ray sources associated with
the young stars in this galaxy.

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