The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A*
Author:
Affiliation:
1. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
2. Department of Astronomy, Columbia University, 550 W 120th St, New York, NY 10027, USA
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/478/4/5209/25102204/sty1261.pdf
Reference116 articles.
1. Sagittarius A* Polarization: No Advection-dominated Accretion Flow, Low Accretion Rate, and Nonthermal Synchrotron Emission
2. Simultaneous Multiwavelength Observations of Sagittarius A*
3. ChandraX‐Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy
4. Instability, turbulence, and enhanced transport in accretion disks
5. PARTICLE ACCELERATION AND THE ORIGIN OF X-RAY FLARES IN GRMHD SIMULATIONS OF SGR A*
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