NONTHERMAL RADIATION OF YOUNG SUPERNOVA REMNANTS: THE CASE OF RX J1713.7−3946
By V. Zirakashvili, F. Aharonian. 2010
175 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ac84a7aa43243cc91e99fd13ceacabaa515383a4
How researchers see this paper
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In Astronomy and Astrophysics
- A. Spitkovsky
- E. Orlando
- D. Caprioli
- Y. Fukui
- Troy A. Porter
- Tsuyoshi Inoue
- Igor V. Moskalenko
- S. Inutsuka
In Nuclear and High Energy Physics
- E. Orlando
- A. Spitkovsky
- D. Caprioli
- Troy A. Porter
- I. Grenier
- Y. Fukui
- Tsuyoshi Inoue
- Igor V. Moskalenko
Citations in the corpus
- OBSERVATIONS OF THE YOUNG SUPERNOVA REMNANT RX J1713.7−3946 WITH THE FERMI LARGE AREA TELESCOPE (2011, background): “7−3946 has been a matter314 of active debate (see Zirakashvili & Aharonian 2010, and references therein).”
- TOWARD UNDERSTANDING THE COSMIC-RAY ACCELERATION AT YOUNG SUPERNOVA REMNANTS INTERACTING WITH INTERSTELLAR CLOUDS: POSSIBLE APPLICATIONS TO RX J1713.7−3946 (2011, background): “These two effects on the thermal X-ray line emission were pointed out in Zirakashvili & Aharonian (2010).”
- SIMULATIONS OF ION ACCELERATION AT NON-RELATIVISTIC SHOCKS. I. ACCELERATION EFFICIENCY (2013, methodology): “…by solving the CR transport equation either numerically (e.g., Berezhko & Völk 1997, 2004; Kang & Jones 1997; Kang et al. 2002; Kang & Jones 2006; Zirakashvili & Aharonian 2010), or analytically (Malkov 1997; Blasi 2002; Amato & Blasi 2006; Caprioli et al. 2010a; Caprioli 2012, and references…”
- Strong evidence for hadron acceleration in Tycho’s supernova remnant (2011, background): “7-3946, which for many years has been regarded as the best candidate as a hadron accelerator due to its brightness in the TeV band (see e.g. Morlino, Amato & Blasi, 2009; Zirakashvili & Aharonian, 2010).”