Understanding Galaxy Formation with ISO Deep Surveys

Understanding Galaxy Formation with ISO Deep Surveys
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通过 ISO 深度巡天了解星系的形成

DOI:
10.1007/s11214-005-8060-3
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发表时间:
2005
影响因子:
10.3
通讯作者:
D. Elbaz
D. Elbaz
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
D. Elbaz

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我们展示通过各种 ISO 河外深部调查获得的结果。尽管IRAS揭示了本地宇宙中存在以数十(LIRG)甚至数百(ULIRG)太阳质量的星系形成恒星的星系,但ISO不仅发现这些星系已经在红移1处就位,而且还发现它们并不是我们曾经认为的极端天体。相反,它们似乎在塑造当今星系方面发挥着主导作用,这从它们在恒星形成的宇宙历史中的作用以及产生 COBE 卫星在远红外到亚毫米范围内检测到的宇宙红外背景中的作用反映出来。
We present the results obtained through the various ISO extragalactic deep surveys. Although IRAS revealed the existence of galaxies forming stars at a rate of a few tens (LIRGs) or even hundreds (ULIRGs) solar masses in the local universe, ISO not only discovered that these galaxies were already in place at redshift one, but also that they are not the extreme objects that we once believed them to be. Instead they appear to play a dominant role in shaping present-day galaxies as reflected by their role in the cosmic history of star formation and in producing the cosmic infrared background detected by the COBE satellite in the far infrared to sub-millimeter range.
DOI: --
发表时间: 2004
期刊: Astronomy and Astrophysics 413
影响因子: --
作者:
Kawara;K. ; Matsuhara;H. ; Okuda;H. ; Taniguchi;Y. ; Sato,Y. ; Sofue;Y. ; Wakamatsu;K. ; Oyabu;S. ; Sanders;D.B. ; Cowie;L.L.
通讯作者: L.L.