中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Stellar Mass and Stellar Mass-to-light Ratio-Color Relations for Low Surface Brightness Galaxies

文献类型:期刊论文

作者Du, Wei1,2; Cheng, Cheng3; Zheng, Zheng1,4; Wu, Hong1,2
刊名ASTRONOMICAL JOURNAL
出版日期2020-04-01
卷号159期号:4页码:17
ISSN号0004-6256
关键词Low surface brightness galaxies Mass-to-light ratio Surface photometry Galaxy masses
DOI10.3847/1538-3881/ab6efb
英文摘要We estimate the stellar mass for a sample of low surface brightness galaxies (LSBGs) by fitting their multiband spectral energy distributions (SEDs) to the stellar population synthesis model. The derived stellar masses (log M-*/M
WOS关键词GIANT BRANCH STARS ; DIGITAL SKY SURVEY ; POPULATION SYNTHESIS ; HI OBSERVATIONS ; LOCAL UNIVERSE ; SIMPLE-MODEL ; EVOLUTION ; I. ; LUMINOSITY ; PHOTOMETRY
资助项目National Natural Science Foundation of China (NSFC)[U1931109] ; National Natural Science Foundation of China (NSFC)[11733006] ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; NSFC[11733006] ; NSFC[11803044] ; NSFC[11933003] ; NSFC[11988101] ; NSFC[11703036] ; NSFC[U1931110] ; NAOC ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS Interdisciplinary Innovation Team[JCTD-2019-05] ; CAS Key Laboratory of FAST ; Chinese Academy of Sciences ; National Key R&D Program of China[2017YFA0402704]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000518990400001
资助机构National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; NSFC ; NSFC ; NAOC ; NAOC ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; CAS Key Laboratory of FAST ; CAS Key Laboratory of FAST ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; 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) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; NSFC ; NSFC ; NAOC ; NAOC ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; CAS Key Laboratory of FAST ; CAS Key Laboratory of FAST ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; 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) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; NSFC ; NSFC ; NAOC ; NAOC ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; CAS Key Laboratory of FAST ; CAS Key Laboratory of FAST ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; 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) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; NSFC ; NSFC ; NAOC ; NAOC ; Chinese Academy of Sciences (CAS) ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; CAS Key Laboratory of FAST ; CAS Key Laboratory of FAST ; Chinese Academy of Sciences ; Chinese Academy of Sciences ; National Key R&D Program of China ; National Key R&D Program of China
源URL[http://ir.bao.ac.cn/handle/114a11/54450]  
专题中国科学院国家天文台
通讯作者Du, Wei
作者单位1.Chinese Acad Sci NAOC, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
2.NAOC, Key Lab Opt Astron, 20A Datun Rd, Beijing 100012, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, South Amer Ctr Astron, Beijing 100101, Peoples R China
4.Chinese Acad Sci, NAOC, Key Lab FAST, 20A Datun Rd, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Du, Wei,Cheng, Cheng,Zheng, Zheng,et al. Stellar Mass and Stellar Mass-to-light Ratio-Color Relations for Low Surface Brightness Galaxies[J]. ASTRONOMICAL JOURNAL,2020,159(4):17.
APA Du, Wei,Cheng, Cheng,Zheng, Zheng,&Wu, Hong.(2020).Stellar Mass and Stellar Mass-to-light Ratio-Color Relations for Low Surface Brightness Galaxies.ASTRONOMICAL JOURNAL,159(4),17.
MLA Du, Wei,et al."Stellar Mass and Stellar Mass-to-light Ratio-Color Relations for Low Surface Brightness Galaxies".ASTRONOMICAL JOURNAL 159.4(2020):17.

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。