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Title: Warped circumbinary disks in active galactic nuclei

Abstract

We study a warping instability of a geometrically thin, non-self-gravitating disk surrounding binary supermassive black holes on a circular orbit. Such a circumbinary disk is subject to not only tidal torques due to the binary gravitational potential but also radiative torques due to radiation emitted from an accretion disk around each black hole. We find that a circumbinary disk initially aligned with the binary orbital plane is unstable to radiation-driven warping beyond the marginally stable warping radius, which is sensitive to both the ratio of vertical to horizontal shear viscosities and the mass-to-energy conversion efficiency. As expected, the tidal torques give no contribution to the growth of warping modes but tend to align the circumbinary disk with the orbital plane. Since the tidal torques can suppress the warping modes in the inner part of circumbinary disk, the circumbinary disk starts to be warped at radii larger than the marginally stable warping radius. If the warping radius is of the order of 0.1 pc, a resultant semi-major axis is estimated to be of the order of 10{sup –2} pc to 10{sup –4} pc for 10{sup 7} M{sub ☉} black hole. We also discuss the possibility that the central objects of observedmore » warped maser disks in active galactic nuclei are binary supermassive black holes with a triple disk: two accretion disks around the individual black holes and one circumbinary disk surrounding them.« less

Authors:
; ; ;  [1];  [2];  [3]
  1. Korea Astronomy and Space Science Institute, Daedeokdaero 776, Yuseong, Daejeon 305-348 (Korea, Republic of)
  2. Faculty of Engineering, Hokkai-Gakuen University, Toyohira-ku, Sapporo 062-8605 (Japan)
  3. Faculty of Management Information, Yamanashi Gakuin University, Kofu, Yamanashi 400-8575 (Japan)
Publication Date:
OSTI Identifier:
22365569
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 790; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCRETION DISKS; BINARY STARS; BLACK HOLES; EFFICIENCY; EMISSION; ENERGY CONVERSION; GALAXIES; GALAXY NUCLEI; GRAVITATIONAL WAVES; INSTABILITY; MASERS; MASS; ORBITS; QUASARS

Citation Formats

Hayasaki, Kimitake, Sohn, Bong Won, Jung, Taehyun, Zhao, Guangyao, Okazaki, Atsuo T., and Naito, Tsuguya, E-mail: kimi@kasi.re.kr. Warped circumbinary disks in active galactic nuclei. United States: N. p., 2014. Web. doi:10.1088/0004-637X/790/1/62.
Hayasaki, Kimitake, Sohn, Bong Won, Jung, Taehyun, Zhao, Guangyao, Okazaki, Atsuo T., & Naito, Tsuguya, E-mail: kimi@kasi.re.kr. Warped circumbinary disks in active galactic nuclei. United States. doi:10.1088/0004-637X/790/1/62.
Hayasaki, Kimitake, Sohn, Bong Won, Jung, Taehyun, Zhao, Guangyao, Okazaki, Atsuo T., and Naito, Tsuguya, E-mail: kimi@kasi.re.kr. 2014. "Warped circumbinary disks in active galactic nuclei". United States. doi:10.1088/0004-637X/790/1/62.
@article{osti_22365569,
title = {Warped circumbinary disks in active galactic nuclei},
author = {Hayasaki, Kimitake and Sohn, Bong Won and Jung, Taehyun and Zhao, Guangyao and Okazaki, Atsuo T. and Naito, Tsuguya, E-mail: kimi@kasi.re.kr},
abstractNote = {We study a warping instability of a geometrically thin, non-self-gravitating disk surrounding binary supermassive black holes on a circular orbit. Such a circumbinary disk is subject to not only tidal torques due to the binary gravitational potential but also radiative torques due to radiation emitted from an accretion disk around each black hole. We find that a circumbinary disk initially aligned with the binary orbital plane is unstable to radiation-driven warping beyond the marginally stable warping radius, which is sensitive to both the ratio of vertical to horizontal shear viscosities and the mass-to-energy conversion efficiency. As expected, the tidal torques give no contribution to the growth of warping modes but tend to align the circumbinary disk with the orbital plane. Since the tidal torques can suppress the warping modes in the inner part of circumbinary disk, the circumbinary disk starts to be warped at radii larger than the marginally stable warping radius. If the warping radius is of the order of 0.1 pc, a resultant semi-major axis is estimated to be of the order of 10{sup –2} pc to 10{sup –4} pc for 10{sup 7} M{sub ☉} black hole. We also discuss the possibility that the central objects of observed warped maser disks in active galactic nuclei are binary supermassive black holes with a triple disk: two accretion disks around the individual black holes and one circumbinary disk surrounding them.},
doi = {10.1088/0004-637X/790/1/62},
journal = {Astrophysical Journal},
number = 1,
volume = 790,
place = {United States},
year = 2014,
month = 7
}
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