UGC 10683B - A possible X-ray emitting Seyfert galaxy

Details UGC 10683B - A possible X-ray emitting Seyfert galaxy UGC 10683B - A possible X-ray emitting Seyfert galaxy

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86.1289w&link_type=abstract

Astronomical Journal, vol. 86, Sept. 1981, p. 1289-1293.

Astronomy and Astrophysics

Astronomy

6

Interacting Galaxies, Seyfert Galaxies, X Ray Sources, Emission Spectra, High Resolution, Light (Visible Radiation)

Scientific paper

Optical spectra are presented for both members of the pair of interacting galaxies UGC 10683, lying close to the HEAO-A1 satellite's unidentified, high-altitude X-ray source 1H 1703-01. It is determined that one galaxy of the pair, UGC 10683B, is of Seyfert Type I, and it is suggested that it may be related to the X-ray source. Higher-resolution X-ray observations are deemed necessary to determine whether there is an identity between UGC 10683B and 1H 1703-01.

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