ACHANDRAVIEW OF NON-THERMAL EMISSION IN THE NORTHWESTERN REGION OF SUPERNOVA REMNANT RCW 86: PARTICLE ACCELERATION AND MAGNETIC FIELDS-Reference-Cited by-同舟云学术

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ACHANDRAVIEW OF NON-THERMAL EMISSION IN THE NORTHWESTERN REGION OF SUPERNOVA REMNANT RCW 86: PARTICLE ACCELERATION AND MAGNETIC FIELDS

Published:2013-11-25 Issue:1 Volume:779 Page:49
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Castro Daniel,Lopez Laura A.,Slane Patrick O.,Yamaguchi Hiroya,Ramirez-Ruiz Enrico,Figueroa-Feliciano Enectali

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/779/i=1/a=49/pdf

Reference50 articles.

1. Detection of TeVγ-ray emission from the shell-type supernova remnant RX J0852.0-4622 with HESS

2. DISCOVERY OF GAMMA-RAY EMISSION FROM THE SHELL-TYPE SUPERNOVA REMNANT RCW 86 WITH HESS

3. High-energy particle acceleration in the shell of a supernova remnant

4. Parameterization of the Chandra point spread function

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1. Turbulent Cosmic Ray–Mediated Shocks in the Hot Ionized Interstellar Medium;The Astrophysical Journal;2022-06-01

2. Gamma-Ray Emission Revealed at the Western Edge of SNR G344.7–0.1;The Astrophysical Journal;2020-11-26

3. Middle-Aged and Old Supernova Remnants;Astronomy and Astrophysics Library;2020

4. Stellar binaries that survive supernovae;Monthly Notices of the Royal Astronomical Society;2019-03-14

5. 2FHL J0826.1–4500: Discovery of a Possible Shock–Cloud Interaction on the Western Edge of the Vela Supernova Remnant;The Astrophysical Journal;2019-01-03

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