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2014MNRAS.440.1125A - Mon. Not. R. Astron. Soc., 440, 1125-1137 (2014/May-2)
Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericentre.
ABARCA D., SADOWSKI A. and SIRONI L.
Abstract (from CDS):
Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)
Journal keyword(s): accretion, accretion discs - black hole physics - methods: numerical
Simbad objects: 3
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