Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericentre

Monthly Notices of the Royal Astronomical Society

Volumn 440, Issue 2, 2014, Pages 1125-1137

  Abarca, David ^a   Sa̧dowski, Aleksander ^a   Sironi, Lorenzo ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Accretion, accretion discs; Black hole physics; Methods: numerical

Indexed keywords

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; BLUE-SHIFTED; CENTERS-OF-MASS; CLOUD DENSITY; COUNTER ROTATING; DYNAMICAL INTERACTIONS; HYDRODYNAMIC SIMULATION; METHOD: NUMERICAL;

NUMERICAL METHODS;

EID: 84898944572     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu244     Document Type: Article

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