Two-dimensional radiation-hydrodynamic model for supercritical disk accretion flows onto neutron stars

Publications of the Astronomical Society of Japan

Volumn 59, Issue 5, 2007, Pages 1033-1041

  Ohsuga, Ken ^a,b  

^a RIKKYO UNIVERSITY   (Japan)

^b INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

Author keywords

Accretion, accretion disks; Hydrodynamics; ISM: jets and outflows; Stars: individual (SS 433); Stars: neutron

Indexed keywords

KINETIC ENERGY; KINETICS; LUMINANCE; NEUTRON IRRADIATION; NEUTRONS; STARS;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; ISM JETS AND OUTFLOWS; NEUTRON STARS; RADIATION FORCES; STAR: INDIVIDUAL (SS 433); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: NEUTRONS; SUPERCRITICAL; TWO-DIMENSIONAL;

HYDRODYNAMICS;

EID: 36849039947     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/59.5.1033     Document Type: Article

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