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Simulations of the origin and fate of the Galactic Center cloud G2

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TLDR
In this paper, the authors investigate the origin and fate of the recently discovered gas cloud G2 close to the Galactic Center and investigate the dynamical evolution of the cloud in combination with currently available observations.
Abstract
We investigate the origin and fate of the recently discovered gas cloud G2 close to the Galactic Center. Our hydrodynamical simulations focussing on the dynamical evolution of the cloud in combination with currently available observations favour two scenarios: a Compact Cloud which started around the year 1995 and an extended Spherical Shell of gas, with an apocenter distance within the disk(s) of young stars. The former is able to explain the detected signal of G2 in the position-velocity-diagram of the year 2008.5 and 2011.5 data. The latter can account for both, G2's signal as well as the fainter extended tail-like structure G2t seen at larger distances to the black hole and smaller velocities. From these first idealised simulations we expect a rise of the current activity of Sgr A* shortly after the closest approach and a constant feeding through a nozzle-like structure over a long period. The near future evolution of the cloud will be a sensitive probe of the conditions of the gas distribution in the milli-parsec environment of the massive black hole in the Galactic Center and will also give us invaluable information of the feeding of black holes and the activation of the central source.

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References
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Journal ArticleDOI

Advection-dominated Accretion: A Self-similar Solution

TL;DR: In this article, the authors consider viscous rotating accretion flows in which most of the viscously dissipated energy is stored as entropy rather than being radiated, and obtain a family of self-similar solutions where the temperature of the accreting gas is nearly virial and the flow is quasi-spherical.
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Monitoring stellar orbits around the Massive Black Hole in the Galactic Center

TL;DR: In this paper, the authors present the results of 16 years of monitoring stellar orbits around the massive black hole in the center of the Milky Way, using high-resolution near-infrared techniques.
Journal ArticleDOI

On the fate of gas accreting at a low rate on to a black hole

TL;DR: In this paper, it was shown that only a small fraction of the gas supplied actually falls on to the black hole, and that the binding energy it releases is transported radially outward by the torque so as to drive away the remainder in the form of a wind.
Journal ArticleDOI

PLUTO: A Numerical Code for Computational Astrophysics

TL;DR: PLUTO as mentioned in this paper is a multiphysics, multialgorithm modular environment particularly oriented toward the treatment of astrophysical flows in presence of discontinuities, and it exploits a general framework for integrating a system of conservation laws, built on modern Godunov-type shockcapturing schemes.
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