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  1. 010 学術雑誌論文
  2. 池内, 了 / IKEUCHI, Satoru

Formation of quasar nuclei in the hearts of ultraluminous infrared galaxies

https://ir.soken.ac.jp/records/3519
https://ir.soken.ac.jp/records/3519
177b9b6e-e21a-4aac-8f74-c1eba06a188c
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1538-4357_514_1_L9.pdf 1538-4357_514_1_L9 (61.8 kB)
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Item type 学術雑誌論文 / Journal Article(1)
公開日 2013-04-25
タイトル
タイトル Formation of quasar nuclei in the hearts of ultraluminous infrared galaxies
タイトル
タイトル Formation of quasar nuclei in the hearts of ultraluminous infrared galaxies
言語 en
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
著者 TANIGUCHI, Yoshiaki

× TANIGUCHI, Yoshiaki

TANIGUCHI, Yoshiaki

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IKEUCHI, Satoru

× IKEUCHI, Satoru

IKEUCHI, Satoru

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SHIOYA, Yasuhiro

× SHIOYA, Yasuhiro

SHIOYA, Yasuhiro

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著者別名 池内, 了

× 池内, 了

池内, 了

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内容記述タイプ Abstract
内容記述 We investigate whether or not supermassive black holes (SMBHs) with mass ≳ 108 M⊙ can be made in the hearts of ultraluminous infrared galaxies (ULIGs) during the course of mergers between/among gas-rich galaxies. (1) If one progenitor galaxy had a seed SMBH with mass of ∼107 M⊙, this seed SMBH can grow up to ≳108 M⊙ due to efficient Bondi-type gas accretion during the course of merger, given a gas density in the circumnuclear region of nH ∼ 103 cm-3. (2) Even if there was no progenitor galaxy with a seed SMBH, star clusters with compact remnants (neutron stars and/or black holes) produced in the circumnuclear starbursts can merge into the merger center within a dynamical timescale of ∼109 yr to form an SMBH with ≳108 M⊙. Note, however, that the contribution of compact remnants supplied from hidden star clusters is necessary to lead to the formation of an SMBH. In conclusion, the ULIGs observed in the local universe can make SMBHs in their centers during the course of merging either by gas accretion onto a seed SMBH or by dynamical relaxation of compact remnants made in the violent circumnuclear starbursts. Therefore, it is quite likely that the ULIGs will finally evolve to optically luminous quasars, as suggested by Sanders et al.
書誌情報 Astrophysical Journal Letters
en : Astrophysical Journal Letters

巻 514, 号 1 PART 2, p. L9-L12, 発行日 1999-03
出版者
出版者 IOP Publishing
ISSN
収録物識別子タイプ ISSN
収録物識別子 20418205
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 http://doi.org/10.1086/311931
関連名称 10.1086/311931
権利
権利情報 © 1999. The American Astronomical Society.
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識別子タイプ URI
関連識別子 http://iopscience.iop.org/page/copyright_notice
関連名称 Copyright
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内容記述タイプ Other
内容記述 application/pdf
著者版フラグ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
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