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Time lags between starburst and AGN activity in galaxy mergers
Published online by Cambridge University Press: 22 May 2014
Abstract
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We show that the observed time lag between starburst and AGN activity can be explained by a viscous time lag the gas needs to flow through the AGN's accretion disk before reaching the central black hole. Our calculations reproduce the observed time lag and are in agreement with the observed correlation between black hole mass and stellar velocity dispersion.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S303: The Galactic Center: Feeding and Feedback in a Normal Galactic Nucleus , October 2013 , pp. 379 - 381
- Copyright
- Copyright © International Astronomical Union 2014
References
Scannapieco, C., Tissera, P. B., White, S. D. M., & Springel, V. 2005, MNRAS 364, 552CrossRefGoogle Scholar