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F07164+5301: An ESB source with WR features
Huang, JH; Gu, QS; Su, HJ; Shang, ZH
1996
Source PublicationASTROPHYSICS AND SPACE SCIENCE
ISSN0004-640X
Volume235Issue:1Pages:109-116
AbstractWe 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 4686, NV lambda lambda 4605-4619 NIII lambda lambda 4634-41, and possibly, CIII lambda lambda 4647-52 emission. The narrow nebular lines are clearly discernable on our spectrum. The number of WR stars derived from the luminosity of HeII lambda 4686 is about 8100. The oxygen abundance is about 9.06 x 10(-4), greater than the solar value.
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordEMISSION-LINE SPECTRA ; WOLF-RAYET GALAXIES ; CLASSIFICATION ; CATALOG ; SAMPLE
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:A1996UG56200010
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8468
Collection期刊(老文献)
Affiliation1.PURPLE MT OBSERV,NANJING 210008,PEOPLES R CHINA
2.CHINESE ACAD SCI,UNITED LAB OPT ASTRON,BEIJING 100080,PEOPLES R CHINA
Recommended Citation
GB/T 7714
Huang, JH,Gu, QS,Su, HJ,et al. F07164+5301: An ESB source with WR features[J]. ASTROPHYSICS AND SPACE SCIENCE,1996,235(1):109-116.
APA Huang, JH,Gu, QS,Su, HJ,&Shang, ZH.(1996).F07164+5301: An ESB source with WR features.ASTROPHYSICS AND SPACE SCIENCE,235(1),109-116.
MLA Huang, JH,et al."F07164+5301: An ESB source with WR features".ASTROPHYSICS AND SPACE SCIENCE 235.1(1996):109-116.
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