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

Astronomy and Astrophysics

Volumn 486, Issue 3, 2008, Pages 679-682

  Bednarek, W ^a   Wagner, R M ^b  

^a UNIVERSITY OF LODZ   (Poland)

^b MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

Author keywords

BL lacertae objects: individual: Mrk 501; Galaxies: active; Gamma rays: theory; Radiation mechanisms: Non thermal

Indexed keywords

ELECTROMAGNETIC WAVES; GAMMA RAYS; HIGH ENERGY PHYSICS; IMAGING TECHNIQUES; IONIZING RADIATION; OPTICAL INSTRUMENTS; OPTICAL TELESCOPES; PHOTOGRAPHY; STARS; TELESCOPES; TELLURIUM COMPOUNDS;

ARRIVAL TIMES; CHERENKOV TELESCOPES; COMPTON; FLARE OBSERVATIONS; GAMMA RAY LARGE AREA SPACE TELESCOPE (GLAST); HIGH ENERGIES; HIGH ENERGY GAMMA RAYS; LOWER ENERGIES; RELATIVISTIC ELECTRONS; TIME-SCALES;

SPACECRAFT OBSERVATORIES;

EID: 47749120966     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079068     Document Type: Article

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