NAOC Open IR  > 光学天文研究部
Mira Variable Stars from LAMOST DR4 Data: Emission Features, Temperature Types, and Candidate Selection
Yao, Yuhan1,2; Liu, Chao3; Deng, Licai3; de Grijs, Richard1,2,4; Matsunaga, Noriyuki5
2017-09-01
Source PublicationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume232Issue:1
AbstractBased on an extensive spectral study of a photometrically confirmed sample of Mira variables, we find a relationship between the relative Balmer emission-line strengths and spectral temperatures of O-rich Mira stars. TheF(H delta)/F-H gamma flux ratio increases from less than unity to five as stars cool down from M0 to M10, which is likely driven by increasing TiO absorption above the deepest shock-emitting regions. We also discuss the relationship between the equivalent widths of the Balmer emission lines and the photometric luminosity phase of our Mira sample stars. Using our 291 Mira spectra as templates for reference, 191 Mira candidates are newly identified from the LAMOST DR4 catalog. We summarize the criteria adopted to select Mira candidates based on emission-line indices and molecular absorption bands. This enlarged spectral sample of Mira variables has the potential to contribute significantly to our knowledge of the optical properties of Mira stars and will facilitate further studies of these late-type, long-period variables.
SubtypeArticle
KeywordCatalogs Stars: Agb And post-Agb Stars: Late-type Stars: Statistics Surveys
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Key Basic Research Program of China(2014CB845700) ; National Key Basic Research Program of China(2014CB845700) ; National Natured Science Foundation of China (NSFC)(11373032 ; National Natured Science Foundation of China (NSFC)(11373032 ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; NSFC(U1631102 ; NSFC(U1631102 ; National Development and Reform Commission ; National Development and Reform Commission ; 11333003) ; 11333003) ; 11373010 ; 11373010 ; 11633005) ; 11633005) ; National Key Basic Research Program of China(2014CB845700) ; National Key Basic Research Program of China(2014CB845700) ; National Natured Science Foundation of China (NSFC)(11373032 ; National Natured Science Foundation of China (NSFC)(11373032 ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; NSFC(U1631102 ; NSFC(U1631102 ; National Development and Reform Commission ; National Development and Reform Commission ; 11333003) ; 11333003) ; 11373010 ; 11373010 ; 11633005) ; 11633005)
DOI10.3847/1538-4365/aa88a9
WOS KeywordSHOCK-INDUCED VARIABILITY ; SIO MASER SURVEY ; GALACTIC BULGE ; DATA RELEASE ; SPECTRAL CLASSIFICATION ; LINES ; WAVES ; GIANTS ; MODELS ; SYSTEM
Indexed BySCI
Language英语
Funding OrganizationNational Key Basic Research Program of China(2014CB845700) ; National Key Basic Research Program of China(2014CB845700) ; National Natured Science Foundation of China (NSFC)(11373032 ; National Natured Science Foundation of China (NSFC)(11373032 ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; NSFC(U1631102 ; NSFC(U1631102 ; National Development and Reform Commission ; National Development and Reform Commission ; 11333003) ; 11333003) ; 11373010 ; 11373010 ; 11633005) ; 11633005) ; National Key Basic Research Program of China(2014CB845700) ; National Key Basic Research Program of China(2014CB845700) ; National Natured Science Foundation of China (NSFC)(11373032 ; National Natured Science Foundation of China (NSFC)(11373032 ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; Hui-Chun Chin and Tsung-Dao Lee Chinese Undergraduate Research Endowment (CURE) ; NSFC(U1631102 ; NSFC(U1631102 ; National Development and Reform Commission ; National Development and Reform Commission ; 11333003) ; 11333003) ; 11373010 ; 11373010 ; 11633005) ; 11633005)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000411593900002
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20116
Collection光学天文研究部
Affiliation1.Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Lu 5, Beijing 100871, Peoples R China
2.Peking Univ, Dept Astron, Yi He Yuan Lu 5, Beijing 100871, Peoples R China
3.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
4.Int Space Sci Inst Beijing, 1 Nanertiao, Beijing 100190, Peoples R China
5.Univ Tokyo, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
Recommended Citation
GB/T 7714
Yao, Yuhan,Liu, Chao,Deng, Licai,et al. Mira Variable Stars from LAMOST DR4 Data: Emission Features, Temperature Types, and Candidate Selection[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2017,232(1).
APA Yao, Yuhan,Liu, Chao,Deng, Licai,de Grijs, Richard,&Matsunaga, Noriyuki.(2017).Mira Variable Stars from LAMOST DR4 Data: Emission Features, Temperature Types, and Candidate Selection.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,232(1).
MLA Yao, Yuhan,et al."Mira Variable Stars from LAMOST DR4 Data: Emission Features, Temperature Types, and Candidate Selection".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 232.1(2017).
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