Simulations of stellar/pulsar-wind interaction along one full orbit

Astronomy and Astrophysics

Volumn 544, Issue , 2012, Pages

  Bosch Ramon, V ^a   Barkov, M V ^b,c   Khangulyan, D ^d   Perucho, M ^e  

^a DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^c Russian Academy of Sciences   (Russian Federation)

^d JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^e UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Gamma rays: stars; Hydrodynamics; Radiation mechanisms: non thermal; Stars: winds, outflows; X rays: binaries

Indexed keywords

ADAPTIVE MESH REFINEMENT; BINARY SYSTEMS; COMPLEX EFFECTS; DOPPLER; ENERGY EXCHANGES; GAMMA RAYS: STARS; HIGH-ENERGY EMISSIONS; INTERACTION STRUCTURES; LORENTZ FACTOR; MASSIVE STARS; NONTHERMAL; NONTHERMAL EMISSION; ORBITAL MOTIONS; PARTICLE ACCELERATION; PHYSICAL EFFECTS; POTENTIAL SITES; RADIATION MECHANISMS: NONTHERMAL; SHOCK STRUCTURE; STARS: WINDS , OUTFLOWS; STELLAR WIND; TWO-DIMENSION; X-RAYS: BINARIES;

COMPUTER SIMULATION; FLUID DYNAMICS; GAMMA RAYS; HYDRODYNAMICS; NUMERICAL ANALYSIS; PARTICLE ACCELERATORS; WIND;

STARS;

EID: 84864334906     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219251     Document Type: Article

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