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Recent study of emission line star 3G71
Hang, HR; Xia, JP
1998-03-01
Source PublicationCHINESE SCIENCE BULLETIN
ISSN1001-6538
Volume43Issue:6Pages:470-473
AbstractNew spectral observations of 3G71 are presented. The main features of optical spectra which exhibit a lot of forbidden lines and unusual strong H-Balmer emission lines are discussed. Our data, together with its large IRAS infrared color excess and other characteristics, show evidence that the star may be a Herbig Ae/Be star rather than the optical counterpart of Be/X-ray source of 1H2214 + 589.
KeywordBe/x-ray Binary Emission Line Iras Identification Herbig Ae/be Star
Subject AreaScience & Technology - Other Topics
WOS HeadingsScience & Technology
Indexed BySCI
Language英语
WOS Research AreaScience & Technology - Other Topics
WOS SubjectMultidisciplinary Sciences
WOS IDWOS:000073926600009
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11183
Collection院士文集_熊大闰
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Chinese Acad Sci, Joint Lab Opt Astron, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Hang, HR,Xia, JP. Recent study of emission line star 3G71[J]. CHINESE SCIENCE BULLETIN,1998,43(6):470-473.
APA Hang, HR,&Xia, JP.(1998).Recent study of emission line star 3G71.CHINESE SCIENCE BULLETIN,43(6),470-473.
MLA Hang, HR,et al."Recent study of emission line star 3G71".CHINESE SCIENCE BULLETIN 43.6(1998):470-473.
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