A dust-parallax distance of 19 megaparsecs to the supermassive black hole in NGC 4151

被引：0

作者：

Sebastian F. Hönig

Darach Watson

Makoto Kishimoto

Jens Hjorth

机构：

[1] Dark Cosmology Centre,Department of Physics

[2] Niels Bohr Institute,undefined

[3] University of Copenhagen,undefined

[4] Juliane Maries Vej 30,undefined

[5] 2100 Copenhagen Ø,undefined

[6] Denmark,undefined

[7] School of Physics & Astronomy,undefined

[8] University of Southampton,undefined

[9] Southampton SO17 1BJ,undefined

[10] UK,undefined

[11] Faculty of Science,undefined

[12] Kyoto Sangyo University,undefined

[13] Kamigamo-motoyama,undefined

[14] Kita-ku,undefined

[15] Kyoto 603-8555,undefined

[16] Japan,undefined

来源：

Nature | 2014年 / 515卷

关键词：

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学科分类号：

摘要：

A distance measurement based on observations of the hot-dust emitting region of the active galaxy NGC 4151 yields a value of 19 megaparsecs, implying a 1.4-fold increase in the dynamical mass of the galaxy’s central black hole and a corresponding correction to emission line reverberation masses of black holes in other active galactic nuclei if calibrated against NGC 4151′s dynamical mass.

引用

页码：528 / 530

页数：2

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