A magnetohydrodynamic model for multiwavelength flares from Sagittarius A⋆ (I): model and the near-infrared and X-ray flares-Reference-Cited by-同舟云学术

A magnetohydrodynamic model for multiwavelength flares from Sagittarius A⋆ (I): model and the near-infrared and X-ray flares

Published:2017-03-16 Issue:3 Volume:468 Page:2552-2568
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Li Ya-Ping¹²,Yuan Feng¹,Wang Q. Daniel³

Affiliation:

1. Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China

2. Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, China

3. Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA

Funder

Natural Science Foundation of China

Ministry of Science and Technology of China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/468/3/2552/13133837/stx655.pdf

Reference109 articles.

1. Simultaneous HESS and Chandra observations of Sagitarius A$^{\star}$ during an X-ray flare

2. Rapid X-ray flaring from the direction of the supermassive black hole at the Galactic Centre

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

4. PARTICLE ACCELERATION AND THE ORIGIN OF X-RAY FLARES IN GRMHD SIMULATIONS OF SGR A*

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