Which physical parameters can be inferred from the emission variability of relativistic jets?

Astronomy and Astrophysics

Volumn 441, Issue 1, 2005, Pages 103-115

  Mimica, P ^a   Aloy, M A ^a,b   Muller E ^a   Brinkmann, W ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITY OF VALENCIA   (Spain)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Acceleration of particles; Galaxies: BL Lac objects: general; Hydrodynamics; Method: numerical; Radiation mechanisms: non thermal; X rays: general

Indexed keywords

DYNAMICS; GALAXIES; HYDRODYNAMICS; KINETIC ENERGY; NUMERICAL METHODS;

ACCELERATION OF PARTICLES; GALAXIES: BL LAC OBJECTS: GENERAL; RADIATION MECHANISMS: NON THERMAL; X-RAY: GENERAL;

JETS;

EID: 25444455337     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053218     Document Type: Article

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