General relativistic magnetohydrodynamic simulations of accretion on to Sgr A*: how important are radiative losses?-Reference-Cited by-同舟云学术

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General relativistic magnetohydrodynamic simulations of accretion on to Sgr A*: how important are radiative losses?

Published:2012-10-08 Issue:3 Volume:426 Page:1928-1939
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Dibi S.¹,Drappeau S.¹,Fragile P. C.²,Markoff S.¹,Dexter J.³

Affiliation:

1. Astronomical Institute ‘Anton Pannekoek’; University of Amsterdam; Postbus 94249; 1090; GE Amsterdam; the Netherlands

2. Department of Physics and Astronomy; College of Charleston; 66 George Street; Charleston; SC; 29424; USA

3. Theoretical Astrophysics Center and Department of Astronomy; University of California; Berkeley; CA; 94720-3411; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/426/3/1928/3105114/426-3-1928.pdf

Reference63 articles.

1. Detection of Polarized Millimeter and Submillimeter Emission from Sagittarius A*

2. Nonoscillatory Central Difference and Artificial Viscosity Schemes for Relativistic Hydrodynamics

3. Cosmos++: Relativistic Magnetohydrodynamics on Unstructured Grids with Local Adaptive Refinement

4. ChandraX‐Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy

5. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

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3. First Sagittarius A* Event Horizon Telescope Results. VIII. Physical Interpretation of the Polarized Ring;The Astrophysical Journal Letters;2024-03-27

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