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|Type:||Artigo de evento|
|Title:||Formation History Of Supermassive Black Holes In A Viable Cosmological Window|
|Abstract:||We show, performing a viable cosmological window, that only the magneto hydrodynamic (MHD) disk model is capable to explain how an intermediate mass black hole (IMBH) (with masses 103 M) grows unto a supermassive black hole (SMBH) (with masses 107 M). We still calculate the supermassive stars sequence of stability. Those stars, with synthetized helium or oxygen cores, collapse to form IMBHs. In our calculation we show that the primordial stars must have rapid rotation if they are in the stable part of the sequence. © 2007 International Astronomical Union.|
|Appears in Collections:||Unicamp - Artigos e Outros Documentos|
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