F07164+5301 - AN ESB SOURCE WITH WR FEATURES

Authors
HUANG JH GU QS SU HJ SHANG ZH
Citation
Jh. Huang et al., F07164+5301 - AN ESB SOURCE WITH WR FEATURES, Astrophysics and space science, 235(1), 1996, pp. 109-116
Citations number
16
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Astrophysics and space science → ACNP
ISSN journal
0004640X
Volume
235
Issue
1
Year of publication
1996
Pages
109 - 116
Database
ISI
SICI code
0004-640X(1996)235:1<109:F-AESW>2.0.ZU;2-J
Abstract
We report on a new ESB source, as defined by Alien et al. (1991), with Wolf-Rayet (WR) bands in its optical spectrum. The WR bump at lambda lambda 4605-4686 is detected. The bump consists of broad HeII lambda 4 686, NV lambda lambda 4605-4619 NIII lambda lambda 4634-41, and possib ly, CIII lambda lambda 4647-52 emission. The narrow nebular lines are clearly discernable on our spectrum. The number of WR stars derived fr om the luminosity of HeII lambda 4686 is about 8100. The oxygen abunda nce is about 9.06 x 10(-4), greater than the solar value.