中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Infrared spectral energy distributions of z similar to 0.7 star-forming galaxies

文献类型:期刊论文

作者Zheng, Xian Zhong; Dole, Herve; Bell, Eric F.; Le Floc'h, Emeric; Rieke, George H.; Rix, Hans-Walter; Schiminovich, David
刊名ASTROPHYSICAL JOURNAL
出版日期2007-11-20
卷号670期号:1页码:301-312
关键词galaxies : evolution galaxies : starburst infrared : galaxies
ISSN号0004-637X
英文摘要We analyze the infrared ( IR) spectral energy distributions ( SEDs) for 10 mu m < lambda(rest) < 100 mu m for similar to 600 galaxies at z similar to 0.7 in the extended Chandra Deep Field South by stacking their Spitzer 24, 70, and 160 mu m images. We place interesting constraints on the average IR SED shape in two bins: the brightest 25% of z similar to 0.7 galaxies detected at 24 mu m, and the remaining 75% of individually detected galaxies. Galaxies without individual detections at 24 mu m were not well detected at 70 and 160 mu m even through stacking. We find that the average IR SEDs of z similar to 0.7 star- forming galaxies fall within the diversity of z similar to 0 templates. While dust obscuration L-IR/L-UV seems to be only a function of star formation rate (SFR; similar to L-IR + L-UV), not of redshift, the dust temperature of star- forming galaxies ( with SFR similar to 10 M-circle dot yr(-1)) at a given IR luminosity was lower at z similar to 0.7 than today. We suggest an interpretation of this phenomenology in terms of dust geometry: intensely star- forming galaxies at z similar to 0 are typically interacting, and host dense centrally concentrated bursts of star formation and warm dust temperatures. At z similar to 0.7, the bulk of intensely star- forming galaxies are relatively undisturbed spirals and irregulars, and we postulate that they have large amounts of widespread lower density star formation, yielding lower dust temperatures for a given IR luminosity. We recommend which IR SEDs are most suitable for modeling intermediate- redshift galaxies with different SFRs.
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]POLYCYCLIC AROMATIC-HYDROCARBON ; SPITZER-SPACE-TELESCOPE ; ORIGINS DEEP SURVEY ; ARRAY CAMERA IRAC ; GOODS-SOUTH FIELD ; LUMINOUS GALAXIES ; LOCAL UNIVERSE ; VLT/FORS2 SPECTROSCOPY ; MIDINFRARED LUMINOSITY ; EVOLUTION-EXPLORER
收录类别SCI
语种英语
WOS记录号WOS:000250965400022
公开日期2012-02-05
源URL[http://159.226.72.40/handle/332002/2420]  
专题紫金山天文台_天体化学和行星科学实验室
作者单位1.Max Planck Inst Astron, D-69117 Heidelberg, Germany
2.Purple Mt Observ, Nanjing 210008, Peoples R China
3.Univ Paris 11, CNRS, UMR 8617, Inst Astrophys Spatiale, F-91405 Orsay, France
4.Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
5.Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
6.Columbia Univ, Dept Astron, New York, NY 10027 USA
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Zheng, Xian Zhong,Dole, Herve,Bell, Eric F.,et al. Infrared spectral energy distributions of z similar to 0.7 star-forming galaxies[J]. ASTROPHYSICAL JOURNAL,2007,670(1):301-312.
APA Zheng, Xian Zhong.,Dole, Herve.,Bell, Eric F..,Le Floc'h, Emeric.,Rieke, George H..,...&Schiminovich, David.(2007).Infrared spectral energy distributions of z similar to 0.7 star-forming galaxies.ASTROPHYSICAL JOURNAL,670(1),301-312.
MLA Zheng, Xian Zhong,et al."Infrared spectral energy distributions of z similar to 0.7 star-forming galaxies".ASTROPHYSICAL JOURNAL 670.1(2007):301-312.

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来源:紫金山天文台

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