NAOC Open IR
A Sample of Edge-on Hi-rich Low Surface Brightness Galaxy Candidates in the 40% ALFALFA Catalog
He, Min1,2; Wu, Hong1,2; Du, Wei1; Liu, He-yang2,3; Lei, Feng-jie1,2; Zhao, Pin-song1,2; Zhang, Bing-qing1,2
2020-06-01
Source PublicationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
ISSN0067-0049
Volume248Issue:2Pages:11
AbstractLow surface brightness galaxies (LSBGs) are defined as galaxies that are fainter than dark night sky and are important for studying our universe. Particularly, edge-on galaxies are useful for the study of rotational velocity and dynamical properties of galaxies. Hence here we focus on searching for edge-on LSBGs. In order to find these edge-on dim galaxies, a series of effects caused by inclination, including the surface brightness profile, internal extinction, and scale length, have been corrected. In this work, we present a catalog of 281 edge-on LSBG candidates, which are selected from the crossmatch between Sloan Digital Sky Survey Data Release 7 and the 40% ALFALFA catalog. We also present the properties of these edge-on LSBG candidates including the absolute magnitude, central surface brightness,B - Vcolor, scale length, and relative thickness. Our result suggests that the correction of inclination effects is very important for obtaining a complete sample of LSBGs.
KeywordCatalogs Low surface brightness galaxies Galaxies
Funding OrganizationNational Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China
DOI10.3847/1538-4365/ab8ead
WOS KeywordSTAR-FORMATION ; DISC GALAXIES ; PHOTOMETRIC PROPERTIES ; STELLAR POPULATIONS ; INTERSTELLAR-MEDIUM ; OXYGEN ABUNDANCES ; SCALING RELATIONS ; SPIRAL GALAXIES ; SPACE DENSITY ; VIRGO CLUSTER
Language英语
Funding ProjectNational Key R&D Program of China[2017YFA0402704] ; National Natural Science Foundation of China (NSFC)[11733006] ; National Natural Science Foundation of China (NSFC)[11403037] ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC[U1931109] ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China[11803047]
Funding OrganizationNational Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences ; NSFC ; NSFC ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Natural Science Foundation of China ; National Natural Science Foundation of China
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000543887000001
PublisherIOP PUBLISHING LTD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/82962
Collection中国科学院国家天文台
Corresponding AuthorHe, Min
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, 20A Datun Rd, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, 20A Datun Rd, Beijing 100101, Peoples R China
Recommended Citation
GB/T 7714
He, Min,Wu, Hong,Du, Wei,et al. A Sample of Edge-on Hi-rich Low Surface Brightness Galaxy Candidates in the 40% ALFALFA Catalog[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2020,248(2):11.
APA He, Min.,Wu, Hong.,Du, Wei.,Liu, He-yang.,Lei, Feng-jie.,...&Zhang, Bing-qing.(2020).A Sample of Edge-on Hi-rich Low Surface Brightness Galaxy Candidates in the 40% ALFALFA Catalog.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,248(2),11.
MLA He, Min,et al."A Sample of Edge-on Hi-rich Low Surface Brightness Galaxy Candidates in the 40% ALFALFA Catalog".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 248.2(2020):11.
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