Feedback Limits to Maximum Seed Masses of Black Holes
نویسندگان
چکیده
منابع مشابه
Feedback Limits Rapid Growth of Seed Black Holes at High Redshift
Seed black holes formed in the collapse of population III stars have been invoked to explain the presence of supermassive black holes at high redshift. It has been suggested that a seed black hole can grow up to 10M⊙ through highly super-Eddington accretion for a period of ∼ 106∼7 yr between redshift z = 20∼ 24. We studied the feedback of radiation pressure, Compton heating and outflow during t...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2017
ISSN: 2041-8213
DOI: 10.3847/2041-8213/835/2/l36