The first low-mass stars: critical metallicity or dust-to-gas ratio?
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Massive black hole factories: Supermassive and quasi-star formation in primordial halosPreserving chemical signatures of primordial star formation in the first low-mass starsThe formation of the extremely primitive star SDSS J102915+172927 relies on dustPredicting the locations of possible long-lived low-mass first stars: importance of satellite dwarf galaxiesOn the Formation of the First Quasars
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The first low-mass stars: critical metallicity or dust-to-gas ratio?
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im Oktober 2011 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2011
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name
The first low-mass stars: critical metallicity or dust-to-gas ratio?
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The first low-mass stars: critical metallicity or dust-to-gas ratio?
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type
label
The first low-mass stars: critical metallicity or dust-to-gas ratio?
@en
The first low-mass stars: critical metallicity or dust-to-gas ratio?
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prefLabel
The first low-mass stars: critical metallicity or dust-to-gas ratio?
@en
The first low-mass stars: critical metallicity or dust-to-gas ratio?
@nl
P2860
P50
P1476
The first low-mass stars: critical metallicity or dust-to-gas ratio?
@en
P2093
Kazuyuki Omukai
P2860
P304
P356
10.1111/J.1365-2966.2011.19818.X
P407
P577
2011-10-28T00:00:00Z
P818
P819
2012MNRAS.419.1566S