A possible time-delayed brightening of the Sgr A* accretion flow after the pericenter passage of the G2 cloud
Author:
Funder
JSPS KAKENHI
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/69/3/43/17668511/psx015.pdf
Reference36 articles.
1. Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericentre
2. THREE-DIMENSIONAL MOVING-MESH SIMULATIONS OF GALACTIC CENTER CLOUD G2
3. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
4. RADIO AND MILLIMETER MONITORING OF $\mathrm{Sgr}$ A⋆: SPECTRUM, VARIABILITY, AND CONSTRAINTS ON THE G2 ENCOUNTER
5. Dynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear Flow
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