ALMA CO Observations of the Mixed-morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma Rays via Shock–Cloud Interactions-Reference-Cited by-同舟云学术

ALMA CO Observations of the Mixed-morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma Rays via Shock–Cloud Interactions

Published:2021-10-01 Issue:2 Volume:919 Page:123
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Sano H.^ORCID,Yoshiike S.^ORCID,Yamane Y.^ORCID,Hayashi K.^ORCID,Enokiya R.^ORCID,Tokuda K.^ORCID,Tachihara K.^ORCID,Rowell G.^ORCID,Filipović M. D.^ORCID,Fukui Y.^ORCID

Funder

MEXT ∣ Japan Society for the Promotion of Science

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ac0dba/pdf

Reference135 articles.

1. FERMI-LAT STUDY OF GAMMA-RAY EMISSION IN THE DIRECTION OF SUPERNOVA REMNANT W49B

2. Detection of the Characteristic Pion-Decay Signature in Supernova Remnants

3. Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field

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