F07164+5301: an ESB source with WR features

Details F07164+5301: an ESB source with WR features F07164+5301: an ESB source with WR features

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.235..109h&link_type=abstract

Astrophysics and Space Science, Volume 235, Issue 1, pp.109-116

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We report on a new ESB source, as defined by Allenet al. (1991), with Wolf-Rayet (WR) bands in its optical spectrum. The WR bump at λλ4605-4686 is detected. The bump consists of broad HeII λ4686, NVλλ4605-4619, NIIIλλ4634-41, and possibly, CIIIλλ4647-52 emission. The narrow nebular lines are clearly discernable on our spectrum. The number of WR stars derived from the luminosity of HeIIλ4686 is about 8100. The oxygen abundance is about 9.06×10-4, greater than the solar value.

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