A model for delayed emission in a very-high energy gamma-ray flare in Markarian 501

2008/04/30 by W. Bednarek, R. M. Wagner
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Gamma-ray bursts and supernovae #Solar and Space Plasma Dynamics #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079068

published as Astron.Astrophys.486:679-682,2008 · 4 pages, no figures, Astronomy & Astrophysics in press

openalex publication_date 2008/05/27 · arxiv created 2008/06/05 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context. Recently, the MAGIC collaboration reported evidence for a delay in the arrival times of photons of different energies during a γ-ray flare from the blazar Markarian 501 on 2005 July 9.

Citations

• The Black Hole Mass of BL Lacertae Objects from the Stellar Velocity Dispersion of the Host Galaxy
• The physical parameters of Markarian 501 during flaring activity