Relativistic flows in TeV blazars

Amir Levinson

Relativistic flows in TeV blazars

Amir Levinson^*

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Conference article › peer-review

1 Scopus citations

Abstract

Rapid variability of the TeV emission in several blazars implies a central black hole mass M_BH < 10⁸M, appreciably smaller than the values estimated from the M_BH −L_bulg relation, and Doppler factors for the γ-ray emitting fluid much larger than those associated with radio patterns. We discuss the conditions in the central engine required to account for the short timescales and large luminosities observed, and propose some explanations for the inferred kinematics of the source on various scales.

Original language	English
Article number	002
Journal	Proceedings of Science
Volume	63
State	Published - 2008
Event	2008 Workshop on Blazar Variability Across the Electromagnetic Spectrum, BLAZARS 2008 - Palaiseau, France Duration: 22 Apr 2008 → 25 Apr 2008

Funding

Funders	Funder number
Israeli Center for High Energy Astrophysics
Israel Science Foundation

Cite this

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Relativistic flows in TeV blazars

Abstract

Funding

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