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The influence of streaming velocities on the formation of the first stars

ABSTRACT. How, when, and where the first stars formed are fundamental questions regarding the epoch of cosmic dawn. A second-order effect in the fluid equation

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Detalles Bibliográficos
Autores principales: Schauer, Anna T. P. (Autor) , Glover, Simon (Autor) , Klessen, Ralf S. (Autor) , Ceverino, Daniel (Autor)
Formato: Article (Journal)
Lenguaje:inglés
Publicado: [April 2019]
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volumen: 484, Número: 3, Pages: 3510-3521
ISSN:1365-2966
DOI:10.1093/mnras/stz013
Acceso en línea:Verlag, Volltext: https://doi.org/10.1093/mnras/stz013
Verlag, Volltext: https://academic.oup.com/mnras/article/484/3/3510/5289417
Enlace del recurso
Notas de Autor:Anna T.P. Schauer, Simon C.O. Glover, Ralf S. Klessen, Daniel Ceverino
Descripción
Sumario:ABSTRACT. How, when, and where the first stars formed are fundamental questions regarding the epoch of cosmic dawn. A second-order effect in the fluid equation
Notas:Advance access publication 2019 January 14
Gesehen am 23.04.2019
Descripción Física:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz013

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