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 |
推荐引用方式 GB/T 7714 | 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. |
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。