Pursuing the Origin of the Gamma Rays in RX J1713.7-3946 Quantifying the Hadronic and Leptonic Components-Reference-Cited by-同舟云学术

Pursuing the Origin of the Gamma Rays in RX J1713.7-3946 Quantifying the Hadronic and Leptonic Components

Published:2021-07-01 Issue:2 Volume:915 Page:84
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Fukui Yasuo^ORCID,Sano Hidetoshi^ORCID,Yamane Yumiko^ORCID,Hayakawa Takahiro^ORCID,Inoue Tsuyoshi^ORCID,Tachihara Kengo^ORCID,Rowell Gavin^ORCID,Einecke Sabrina^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/abff4a/pdf

Reference61 articles.

1. OBSERVATIONS OF THE YOUNG SUPERNOVA REMNANT RX J1713.7–3946 WITH THEFERMILARGE AREA TELESCOPE

2. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946

3. A joint spectro-imaging analysis of theXMM-Newtonand HESS observations of the supernova remnant RX J1713.7-3946

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

5. Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep HESS observations

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