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- W36990711 abstract "We outline a method to infer the global history of star formation in galaxies from absorption-line observations of quasars. The application to existing data leads to the conclusion that most stars formed at relatively low redshifts ( z ≲ 2). The results obtained by this absorption-based method are consistent with those obtained subsequently by emission-based methods." @default.
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- W36990711 date "2002-01-01" @default.
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- W36990711 title "Global Evolution of the Stars, Gas, Metals, and Dust in Galaxies" @default.
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- W36990711 doi "https://doi.org/10.1017/s0074180900113932" @default.
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