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東京経済大学人文自然科学論集 Journal of Humanities and Natural Sciences >
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Please use this identifier to cite or link to this item: http://hdl.handle.net/11150/1040

Title: 超大質量ブラックホール質量 : バルジ質量関係の進化と銀河形成過程 
Other Titles: On the evolution of the supermassive black hole mass-bulge mass relation : effects of galaxy formation processes
Authors: 榎, 基宏
ENOKI, Motohiro
Abstract: In the local universe, the mass of supermassive black hole (SMBH), MBH, is proportional to the bulge mass of the host galaxy, Mbluge. We investigate effects of galaxy formation processes on the evolution of the MBH−Mbulge relation, using a semianalytic model of galaxy and SMBH formation. We find that the mass ratio MBH/Mbulge decreases with cosmic time. In our model, the mass growth processes of SMBH are cold gas accretion during starburst and SMBHs coalescence. Bulges grow from stars formed from cold gas during starbursts. Moreover, bulges also grow from stars in progenitor galaxies. Because cold gas in galaxies depleted by star formation, the amounts of cold gas accreted onto SMBH decrease with time. On the other hand, bulges grow from stars in progenitor galaxies during mergers, even at low redshifts. As a result, one should expect the MBH−Mbulge relation to evolve with cosmic time. Comparing these results with observations in a future, we can put a stringent constraint on galaxy and SMBH formation model.
journaltitle: 人文自然科学論集 = The Journal of Humanities and Natural Sciences
Issue Date: 5-Dec-2012
Publisher: 東京経済大学人文自然科学研究会
issue: 133
Start Page: 31
End Page: 41
URI: http://hdl.handle.net/11150/1040
ISSN: 0495-8012
Appears in Collections:133号

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