Accretion vs. colliding wind models for the gamma-ray binary LS i + 61 303: An assessment

Astronomy and Astrophysics

Volumn 474, Issue 1, 2007, Pages 15-22

  Romero, G E ^a,b,e   Okazaki, A T ^c   Orellana, M ^a,b,e   Owocki, S P ^d  

^a UNIVERSIDAD NACIONAL DE LA PLATA   (Argentina)

^b INSTITUTO ARGENTINO DE RADIOASTRONOMÍA   (Argentina)

^c Hokkai Gaukuen University   (Japan)

^d UNIVERSITY OF DELAWARE   (United States)

^e Universidad Nacional del Litoral   (Argentina)

Author keywords

Gamma rays: theory; Stars: individual: LS I +61 303; X rays: binaries

Indexed keywords

DATA ACQUISITION; MATHEMATICAL MODELS; ORBITS; STARS; X RAY ANALYSIS;

COMETARY TAIL; PULSAR WINDS; RADIO OBSERVATIONS; SMOOTHED PARTICLE HYDRODYNAMICS;

GAMMA RAYS;

EID: 35348977240     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078035     Document Type: Article

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