机译:高恒星形成率是早期和现代盘状星系湍流的起源
Centre for Astrophysics and Supercomputing, Swinburne University, PO Box 218, Hawthorn, Victoria 3122, Australia;
rnCentre for Astrophysics and Supercomputing, Swinburne University, PO Box 218, Hawthorn, Victoria 3122, Australia;
rnResearch School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston, Australian Capital Territory 2611, Australia;
rnDepartmentof Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto, Ontario M5S3H4, Canada;
rnCentre for Astrophysics and Supercomputing, Swinburne University, PO Box 218, Hawthorn, Victoria 3122, Australia;
rnDepartmentof Astronomy and Astrophysics, University of Toronto, 50 St George Street, Toronto, Ontario M5S3H4, Canada;
rnObservatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, California 91101, USA;
rnAustralian Astronomical Observatory, PO Box 296, Epping, New South Wales 1710, Australia;
rnAustralian Astronomical Observatory, PO Box 296, Epping, New South Wales 1710, Australia;
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机译:贫金属恒星的元素丰度可以追溯到银河系厚盘的起源
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机译:高恒星形成率是早期和现代盘状星系中湍流的起源