Cold streams in early massive hot haloes as the main mode of galaxy formation
Cold streams in early massive hot haloes as the main mode of galaxy formation
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DOI:
10.1038/nature07648
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发表时间:
2008-08
期刊:
影响因子:
64.8
通讯作者:
A. Dekel;Y. Birnboim;G. Engel;J. Freundlich;T. Goerdt;M. Mumcuoglu;E. Neistein;C. Pichon;R. Tey
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文献类型:
--
作者:
A. Dekel;Y. Birnboim;G. Engel;J. Freundlich;T. Goerdt;M. Mumcuoglu;E. Neistein;C. Pichon;R. Tey
The massive galaxies in the young universe, ten billion years ago, formed stars at surprising intensities. 1, 2 While this was commonly attributed to violent mergers, many of these galaxies seem to be extended rotating discs incompatible with mergers. 3, 2, 4 In order to uncover the origin of this phenomenon, we use a state-of-the-art cosmological simulation5 and clustering theory6, 7 to explore how these galaxies acquired their gas. We find that these are “Stream-Fed Galaxies”, growing via steady, narrow, cold gas streams, which penetrate effectively through the shock-heated media of dark-matter haloes as massive as the Milky Way’s. This confirms an earlier conjecture. 8 Half the stream mass is in clumps leading to mergers of mass ratio 1: 10 or higher, and half is in smoother flows. Since the merger duty cycle is 0.1, three-quarters of the galaxies forming stars at a given rate are fed by smooth streams. Unlike destructive major mergers, the smoother flows can keep the discs intact, though thick and perturbed. The observed abundance of star-forming galaxies implies that the inflowing gas turns into stars at maximum efficiency. In contrast, the sub-millimeter galaxies that form stars even more intensely1, 9, 10 are largely compact merger-induced starbursts in haloes twice as massive.