Discovery of Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Kesteven 79-Reference-Cited by-同舟云学术

Discovery of Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Kesteven 79

Published:2018-09-12 Issue:2 Volume:864 Page:161
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Kuriki M.,Sano H.^ORCID,Kuno N.,Seta M.,Yamane Y.^ORCID,Inaba T.,Nagaya T.,Yoshiike S.^ORCID,Okawa K.,Tsutsumi D.,Hattori Y.,Kohno M.,Fujita S.,Nishimura A.,Ohama A.,Matsuo M.,Tsuda Y.,Torii K.^ORCID,Minamidani T.^ORCID,Umemoto T.,Rowell G.^ORCID,Bamba A.^ORCID,Tachihara K.^ORCID,Fukui Y.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/864/i=2/a=161/pdf

Reference65 articles.

1. A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7–3946 with HESS

2. Distinguishing between HII regions and planetary nebulae with Hi-GAL, WISE, MIPSGAL, and GLIMPSE

3. FERMI-LAT OBSERVATIONS OF SUPERNOVA REMNANTS KESTEVEN 79

4. New identification of the mixed-morphology supernova remnant G298.6−0.0 with possible gamma-ray association

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