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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Astrophysics and space science 235 (1996), S. 109-116 
    ISSN: 1572-946X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract 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.
    Type of Medium: Electronic Resource
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