NAOC Open IR  > 光学天文研究部
Molecular Gas and Star-formation in Low Surface Brightness Galaxies
Cao, Tian-Wen1,2,3; Wu, Hong1,2; Du, Wei1; Lei, Feng-Jie1,2; Zhu, Ming1; Wouterloot, Jan4; Parsons, Harriet4; Zhu, Yi-Nan1; Wu, Chao-Jian1; Yang, Fan1; Cao, Chen5; Zhou, Zhi-Min1; He, Min1,2; Jin, Jun-Jie1,2; Wicker, James E.1
2017-09-01
Source PublicationASTRONOMICAL JOURNAL
Volume154Issue:3
AbstractWe have obtained CO(J = 2-1) spectra of nine face-on low surface brightness galaxies using the JCMT 15 m telescope and observed Ha images using the 2.16 m telescope of NAOC. As no CO has been detected, only upper limits on the H-2 masses are given. The upper limits of total molecular hydrogen masses are about (1.2-82.4) x 10(7) M-circle dot. Their star-formation rates are mainly lower than 0.4 M-circle dot yr(-1) and star-formation efficiencies are lower than 1.364 x 10(-10) yr(-1). Our results show that the absence of molecular gas content is the direct reason for the low star-formation rate. The low star -formation efficiency probably resulted from the low efficiency of H I gas transforming to H-2 gas.
SubtypeArticle
KeywordGalaxies: Evolution Galaxies: Star Formation Ism: Molecules
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationNational Natural Science Foundation of China(11403037 ; National Natural Science Foundation of China(11403037 ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; (M15BI057) ; (M15BI057) ; 11733006 ; 11733006 ; 2014CB845705) ; 2014CB845705) ; 11173030 ; 11173030 ; 11225316 ; 11225316 ; 11503013 ; 11503013 ; 11403061 ; 11403061 ; U1531245 ; U1531245 ; 11303038) ; 11303038) ; National Natural Science Foundation of China(11403037 ; National Natural Science Foundation of China(11403037 ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; (M15BI057) ; (M15BI057) ; 11733006 ; 11733006 ; 2014CB845705) ; 2014CB845705) ; 11173030 ; 11173030 ; 11225316 ; 11225316 ; 11503013 ; 11503013 ; 11403061 ; 11403061 ; U1531245 ; U1531245 ; 11303038) ; 11303038)
DOI10.3847/1538-3881/aa845a
WOS KeywordDISK GALAXIES ; INTERSTELLAR-MEDIUM ; SPIRAL GALAXIES ; FORMATION EFFICIENCY ; IRREGULAR GALAXIES ; OXYGEN ABUNDANCES ; CONVERSION FACTOR ; NEARBY GALAXIES ; HI OBSERVATIONS ; FORMATION LAW
Indexed BySCI
Language英语
Funding OrganizationNational Natural Science Foundation of China(11403037 ; National Natural Science Foundation of China(11403037 ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; (M15BI057) ; (M15BI057) ; 11733006 ; 11733006 ; 2014CB845705) ; 2014CB845705) ; 11173030 ; 11173030 ; 11225316 ; 11225316 ; 11503013 ; 11503013 ; 11403061 ; 11403061 ; U1531245 ; U1531245 ; 11303038) ; 11303038) ; National Natural Science Foundation of China(11403037 ; National Natural Science Foundation of China(11403037 ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program, "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; China Ministry of Science and Technology under the State Key Development Program for Basic Research(2012CB821803 ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; (M15BI057) ; (M15BI057) ; 11733006 ; 11733006 ; 2014CB845705) ; 2014CB845705) ; 11173030 ; 11173030 ; 11225316 ; 11225316 ; 11503013 ; 11503013 ; 11403061 ; 11403061 ; U1531245 ; U1531245 ; 11303038) ; 11303038)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000410575200001
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/20135
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.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing, Peoples R China
3.China Chile Joint Ctr Astron, Chinese Acad Sci South Amer Ctr Astron, Camino Observ 1515, Santiago, Chile
4.East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA
5.Shandong Univ Weihai, Sch Space Sci & Phys, Weihai 264209, Shandong, Peoples R China
Recommended Citation
GB/T 7714
Cao, Tian-Wen,Wu, Hong,Du, Wei,et al. Molecular Gas and Star-formation in Low Surface Brightness Galaxies[J]. ASTRONOMICAL JOURNAL,2017,154(3).
APA Cao, Tian-Wen.,Wu, Hong.,Du, Wei.,Lei, Feng-Jie.,Zhu, Ming.,...&Wicker, James E..(2017).Molecular Gas and Star-formation in Low Surface Brightness Galaxies.ASTRONOMICAL JOURNAL,154(3).
MLA Cao, Tian-Wen,et al."Molecular Gas and Star-formation in Low Surface Brightness Galaxies".ASTRONOMICAL JOURNAL 154.3(2017).
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