The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence
文献类型:期刊论文
作者 | Guo, Rui1,2,3; Hao, Cai-Na3; Xia, X. Y.3; Mao, Shude2,4,5,6; Shi, Yong7,8 |
刊名 | Astrophysical journal |
出版日期 | 2016-07-20 |
卷号 | 826期号:1页码:12 |
ISSN号 | 0004-637X |
关键词 | Galaxies: evolution Galaxies: formation Galaxies: interactions Galaxies: starburst Infrared: galaxies |
DOI | 10.3847/0004-637x/826/1/30 |
通讯作者 | Hao, cai-na(cainahao@gmail.com) |
英文摘要 | With the aim of exploring the fast evolutionary path from the blue cloud of star-forming galaxies to the red sequence of quiescent galaxies in the local universe, we select a local advanced merging infrared luminous and ultraluminous galaxy (adv-merger (u)lirgs) sample and perform careful dust extinction corrections to investigate their positions in the star formation rate-m-*, u-r, and nuv-r color-mass diagrams. the sample consists of 89 (u) lirgs at the late merger stage, obtained from cross-correlating the infrared astronomical satellite point source catalog redshift survey and 1 jy ulirgs samples with the sloan digital sky survey dr7 database. our results show that 74% +/- 5% of adv-merger (u) lirgs are localized above the 1 sigma line of the local star-forming galaxy main sequence. we also find that all adv-merger (u) lirgs are more massive than and as blue as the blue cloud galaxies after corrections for galactic and internal dust extinctions, with 95% +/- 2% and 81% +/- 4% of them outside the blue cloud on the u-r and nuv-r color-mass diagrams, respectively. these results, combined with the short timescale for exhausting the molecular gas reservoir in adv-merger (u) lirgs (3 x 10(7) to 3 x 10(8) years), imply that the adv-merger (u) lirgs are likely at the starting point of the fast evolutionary track previously proposed by several groups. while the number density of adv-merger (u) lirgs is only similar to 0.1% of the blue cloud star-forming galaxies in the local universe, this evolutionary track may play a more important role at high redshift. |
WOS关键词 | DIGITAL-SKY-SURVEY ; ULTRALUMINOUS INFRARED GALAXIES ; STAR-FORMING GALAXIES ; COMPACT QUIESCENT GALAXIES ; FORMATION RATE INDICATORS ; COLOR-MAGNITUDE DIAGRAM ; SIMILAR-TO 2 ; EXTRAGALACTIC LEGACY SURVEY ; SUPERMASSIVE BLACK-HOLES ; STELLAR MASS FUNCTIONS |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000381962200030 |
URI标识 | http://www.irgrid.ac.cn/handle/1471x/2374447 |
专题 | 中国科学院大学 |
通讯作者 | Hao, Cai-Na |
作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Tianjin Normal Univ, Tianjin Astrophys Ctr, Tianjin 300387, Peoples R China 4.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 5.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China 6.Univ Manchester, Jodrell Bank Ctr Astrophys, Alan Turing Bldg, Manchester M13 9PL, Lancs, England 7.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China 8.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Guo, Rui,Hao, Cai-Na,Xia, X. Y.,et al. The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence[J]. Astrophysical journal,2016,826(1):12. |
APA | Guo, Rui,Hao, Cai-Na,Xia, X. Y.,Mao, Shude,&Shi, Yong.(2016).The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence.Astrophysical journal,826(1),12. |
MLA | Guo, Rui,et al."The role of major gas-rich mergers on the evolution of galaxies from the blue cloud to the red sequence".Astrophysical journal 826.1(2016):12. |
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来源:中国科学院大学
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