中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A catalog of early-type emission-line stars and H alpha line profiles from LAMOST DR2

文献类型:期刊论文

作者Hou, Wen1,2; Luo, A-Li1,2; Hu, Jing-Yao1; Yang, Hai-Feng1,2,3; Du, Chang-De1,2; Liu, Chao1; Lee, Chien-De4; Lin, Chien-Cheng5; Wang, Yue-Fei6; Zhang, Yong6
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2016-09-01
卷号16期号:9
关键词stars: early-type stars: emission-line, Be stars: pre-main sequence binaries: close
英文摘要We present a catalog including 11 204 spectra of 10 436 early-type emission-line stars from LAMOST DR2, among which 9752 early-type emission-line spectra are newly discovered. For these early type emission-line stars, we discuss the morphological and physical properties of their low-resolution spectra. In this spectral sample, the H alpha emission profiles display a wide variety of shapes. Based on the H alpha line profiles, these spectra are categorized into five distinct classes: single-peak emission, single-peak emission in absorption, double-peak emission, double-peak emission in absorption, and P-Cygni profiles. To better understand what causes the H alpha line profiles, we divide these objects into four types from the perspective of physical classification, which include classical Be stars, Herbig Ae/Be stars, close binaries and spectra contaminated by H (II) regions. The majority of Herbig Ae/Be stars and classical Be stars are identified and separated using a (H-K, K-W1) color-color diagram. We also discuss 31 binary systems that are listed in the SIMBAD on-line catalog and identify 3600 spectra contaminated by H (II) regions after cross-matching with positions in the Dubout-Crillon catalog. A statistical analysis of line profiles versus classifications is then conducted in order to understand the distribution of H alpha profiles for each type in our sample. Finally, we also provide a table of 172 spectra with Fe (II) emission lines and roughly calculate stellar wind velocities for seven spectra with P-Cygni profiles.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]HERBIG-AE/BE STARS ; M IR-EXCESS ; DATA RELEASE ; B STARS ; SPECTROSCOPY ; BALMER ; 2MASS ; DISKS
收录类别SCI
语种英语
WOS记录号WOS:000385995800006
源URL[http://ir.bao.ac.cn/handle/114a11/6895]  
专题国家天文台_光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Taiyuan Univ Sci & Technol, Sch Comp Sci & Technol, Taiyuan 030024, Peoples R China
4.Natl Cent Univ, Inst Astron, Jhongli, Taiwan
5.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
6.Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China
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Hou, Wen,Luo, A-Li,Hu, Jing-Yao,et al. A catalog of early-type emission-line stars and H alpha line profiles from LAMOST DR2[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2016,16(9).
APA Hou, Wen.,Luo, A-Li.,Hu, Jing-Yao.,Yang, Hai-Feng.,Du, Chang-De.,...&Hou, Yong-Hui.(2016).A catalog of early-type emission-line stars and H alpha line profiles from LAMOST DR2.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,16(9).
MLA Hou, Wen,et al."A catalog of early-type emission-line stars and H alpha line profiles from LAMOST DR2".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 16.9(2016).

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来源:国家天文台

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