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Candidate members of the Pal 5, GD-1, Cetus Polar and Orphan tidal stellar halo streams from SDSS DR9, LAMOST DR3 and APOGEE catalogs
Li, Guang-Wei1; Yanny, Brian2; Zhang, Hao-Tong1; Bai, Zong-Rui1; Wu, Yue1; Dong, Yi-Qiao1; Lei, Ya-Juan1; Yuan, Hai-Long1; Hou, Yong-Hui3; Wang, Yue-Fei3; Zhang, Yong3
2017-06-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume17Issue:6
AbstractWe present candidate members of the Pal 5, GD-1, Cetus Polar and Orphan tidal stellar streams found in LAMOST DR3, SDSS DR9 and APOGEE catalogs. In LAMOST DR3, we find 20, 4 and 24 high confidence candidates of tidal streams GD-1, Cetus Polar and Orphan respectively. We also list 59, 118 and 10 high confidence candidates of tidal streams Cetus Polar, Orphan and Pal 5, respectively from the SDSS DR9 spectroscopic catalog. Furthermore, we find seven high confidence candidates of the Pal 5 tidal stream in the APOGEE data. Compared with SDSS, the new candidates from LAMOST DR3 are brighter, so that together, more of the color-magnitude diagram, including the giant branch, can be explored. Analysis of the SDSS data shows that there are three metallicity peaks associated with the Orphan stream which also exhibit some spatial separation. The LAMOST data confirm multiple metallicities in this stream. The metallicity, given by the higher resolution APOGEE instrument, of the Pal 5 tidal stream is [Fe/H] similar to -1.2, higher than that given earlier by SDSS spectra. Many previously unidentified stream members are tabulated here for the first time, along with existing members, allowing future researchers to further constrain the orbits of these objects as they move within the Galaxy's dark matter potential.
SubtypeArticle
KeywordGalaxy: Structure General: Stream Galaxy: Structure Individual (Gd-1 Orphan Cetus Pal 5)
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Natural Science Foundation of China (NSFC)(Y011161001 ; National Natural Science Foundation of China (NSFC)(Y011161001 ; US NSF LAMOST-PLUS grant ; US NSF LAMOST-PLUS grant ; Guangdong Provincial Engineering Technology Research Center for Data Science ; Guangdong Provincial Engineering Technology Research Center for Data Science ; National Development and Reform Commission ; National Development and Reform Commission ; 11403056 ; 11403056 ; 11673036 ; 11673036 ; 11333004) ; 11333004) ; National Natural Science Foundation of China (NSFC)(Y011161001 ; National Natural Science Foundation of China (NSFC)(Y011161001 ; US NSF LAMOST-PLUS grant ; US NSF LAMOST-PLUS grant ; Guangdong Provincial Engineering Technology Research Center for Data Science ; Guangdong Provincial Engineering Technology Research Center for Data Science ; National Development and Reform Commission ; National Development and Reform Commission ; 11403056 ; 11403056 ; 11673036 ; 11673036 ; 11333004) ; 11333004)
DOI10.1088/1674-4527/17/6/62
WOS KeywordDIGITAL SKY SURVEY ; GALACTIC HALO ; SAGITTARIUS ; GALAXY ; STARS ; SPECTROSCOPY ; TELESCOPE ; CLUSTERS ; SEGUE ; ORBIT
Indexed BySCI
Language英语
Funding OrganizationNational Natural Science Foundation of China (NSFC)(Y011161001 ; National Natural Science Foundation of China (NSFC)(Y011161001 ; US NSF LAMOST-PLUS grant ; US NSF LAMOST-PLUS grant ; Guangdong Provincial Engineering Technology Research Center for Data Science ; Guangdong Provincial Engineering Technology Research Center for Data Science ; National Development and Reform Commission ; National Development and Reform Commission ; 11403056 ; 11403056 ; 11673036 ; 11673036 ; 11333004) ; 11333004) ; National Natural Science Foundation of China (NSFC)(Y011161001 ; National Natural Science Foundation of China (NSFC)(Y011161001 ; US NSF LAMOST-PLUS grant ; US NSF LAMOST-PLUS grant ; Guangdong Provincial Engineering Technology Research Center for Data Science ; Guangdong Provincial Engineering Technology Research Center for Data Science ; National Development and Reform Commission ; National Development and Reform Commission ; 11403056 ; 11403056 ; 11673036 ; 11673036 ; 11333004) ; 11333004)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000408362700014
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20140
Collection光学天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
2.Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
3.Chinese Acad Sci, Nanjing Inst Astron Opt & Technol, Natl Astron Observ, Nanjing 210042, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Li, Guang-Wei,Yanny, Brian,Zhang, Hao-Tong,et al. Candidate members of the Pal 5, GD-1, Cetus Polar and Orphan tidal stellar halo streams from SDSS DR9, LAMOST DR3 and APOGEE catalogs[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2017,17(6).
APA Li, Guang-Wei.,Yanny, Brian.,Zhang, Hao-Tong.,Bai, Zong-Rui.,Wu, Yue.,...&Zhang, Yong.(2017).Candidate members of the Pal 5, GD-1, Cetus Polar and Orphan tidal stellar halo streams from SDSS DR9, LAMOST DR3 and APOGEE catalogs.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,17(6).
MLA Li, Guang-Wei,et al."Candidate members of the Pal 5, GD-1, Cetus Polar and Orphan tidal stellar halo streams from SDSS DR9, LAMOST DR3 and APOGEE catalogs".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 17.6(2017).
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