Infrared Spectral Energy Distributions ofz∼ 0.7 Star‐forming Galaxies
نویسندگان
چکیده
منابع مشابه
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Submillimetre (sub-mm) galaxies have very high infrared (IR) luminosities and are thousands of times more numerous at z ∼ 2 than local ultra-luminous IR galaxies. They therefore represent a key phase in galaxy evolution which can be missed in optical surveys. Determining their contribution to the global star formation rate requires dissecting their IR emission into contributions from starbursts...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2007
ISSN: 0004-637X,1538-4357
DOI: 10.1086/520529