Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericentre
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/440/2/1125/18498041/stu244.pdf
Reference30 articles.
1. THREE-DIMENSIONAL MOVING-MESH SIMULATIONS OF GALACTIC CENTER CLOUD G2
2. ChandraX‐Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy
3. HYDRODYNAMICAL SIMULATIONS OF A COMPACT SOURCE SCENARIO FOR THE GALACTIC CENTER CLOUD G2
4. EVIDENCE FOR LOW BLACK HOLE SPIN AND PHYSICALLY MOTIVATED ACCRETION MODELS FROM MILLIMETER-VLBI OBSERVATIONS OF SAGITTARIUS A*
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3. 3D AMR hydrosimulations of a compact-source scenario for the Galactic Centre cloud G2;Monthly Notices of the Royal Astronomical Society;2018-06-01
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