中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
热门
OBSCURED STAR FORMATION IN INTERMEDIATE-DENSITY ENVIRONMENTS: A SPITZER STUDY OF THE ABELL 901/902 SUPERCLUSTER

文献类型:期刊论文

作者Gallazzi, Anna1; Bell, Eric F.1; Wolf, Christian2; Gray, Meghan E.3; Papovich, Casey4; Barden, Marco5; Peng, Chien Y.6; Meisenheimer, Klaus1; Heymans, Catherine7; van Kampen, Eelco5
刊名ASTROPHYSICAL JOURNAL
出版日期2009-01-10
卷号690期号:2页码:1883-1900
关键词galaxies: evolution galaxies: general galaxies: stellar content
ISSN号0004-637X
英文摘要We explore the amount of obscured star formation as a function of environment in the Abell 901/902 (A901/902) supercluster at z = 0.165 in conjunction with a field sample drawn from the A901 and CDFS fields, imaged with the Hubble Space Telescope as part of the Space Telescope A901/902 Galaxy Evolution Survey and Galaxy Evolution from Morphology and Spectral Energy Distributions (SEDs) Survey. We combine the combo-17 near-UV/optical SED with Spitzer 24 mu m photometry to estimate both the unobscured and obscured star formation in galaxies with M(*) > 10(10) M(circle dot). We find that the star formation activity in massive galaxies is suppressed in dense environments, in agreement with previous studies. Yet, nearly 40% of the star-forming (SF) galaxies have red optical colors at intermediate and high densities. These red systems are not starbursting; they have star formation rates (SFRs) per unit stellar mass similar to or lower than blue SF galaxies. More than half of the red SF galaxies have low infrared-to-ultraviolet (IR-to-UV) luminosity ratios, relatively high Sersicindices, and they are equally abundant at all densities. They might be gradually quenching their star formation, possibly but not necessarily under the influence of gas-removing environmental processes. The other greater than or similar to 40% of the red SF galaxies have high IR-to-UV luminosity ratios, indicative of high dust obscuration. They have relatively high specific SFRs and are more abundant at intermediate densities. Our results indicate that while there is an overall suppression in the SF galaxy fraction with density, the small amount of star formation surviving the cluster environment is to a large extent obscured, suggesting that environmental interactions trigger a phase of obscured star formation, before complete quenching.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]HUBBLE-SPACE-TELESCOPE ; EARLY-TYPE GALAXIES ; SPECTRAL ENERGY-DISTRIBUTIONS ; ALPHA SURFACE PHOTOMETRY ; ACTIVE GALACTIC NUCLEI ; DIGITAL SKY SURVEY ; DARK-MATTER HALOS ; VIRGO CLUSTER ; SPIRAL GALAXIES ; STELLAR MASS
收录类别SCI
语种英语
WOS记录号WOS:000262726900071
公开日期2011-12-08
源URL[http://159.226.72.40/handle/332002/1597]  
专题紫金山天文台_星系中的恒星形成研究团组
作者单位1.Max Planck Inst Astron, D-69117 Heidelberg, Germany
2.Univ Oxford, Dept Phys, Oxford OX1 3RH, England
3.Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
4.Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
5.Univ Innsbruck, Inst Astro & Particle Phys, A-6020 Innsbruck, Austria
6.Herzberg Inst Astrophys, NRC, Victoria, BC V9E 2E7, Canada
7.Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
8.European So Observ, Santiago 19, Chile
9.Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
10.Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
推荐引用方式
GB/T 7714
Gallazzi, Anna,Bell, Eric F.,Wolf, Christian,et al. OBSCURED STAR FORMATION IN INTERMEDIATE-DENSITY ENVIRONMENTS: A SPITZER STUDY OF THE ABELL 901/902 SUPERCLUSTER[J]. ASTROPHYSICAL JOURNAL,2009,690(2):1883-1900.
APA Gallazzi, Anna.,Bell, Eric F..,Wolf, Christian.,Gray, Meghan E..,Papovich, Casey.,...&Zheng, Xianzhong.(2009).OBSCURED STAR FORMATION IN INTERMEDIATE-DENSITY ENVIRONMENTS: A SPITZER STUDY OF THE ABELL 901/902 SUPERCLUSTER.ASTROPHYSICAL JOURNAL,690(2),1883-1900.
MLA Gallazzi, Anna,et al."OBSCURED STAR FORMATION IN INTERMEDIATE-DENSITY ENVIRONMENTS: A SPITZER STUDY OF THE ABELL 901/902 SUPERCLUSTER".ASTROPHYSICAL JOURNAL 690.2(2009):1883-1900.

入库方式: OAI收割

来源:紫金山天文台

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。