Hydrodynamic simulations of the interaction of supernova shock waves with a clumpy environment: the case of the RX J0852.0−4622 (Vela Jr) supernova remnant-Reference-Cited by-同舟云学术

Hydrodynamic simulations of the interaction of supernova shock waves with a clumpy environment: the case of the RX J0852.0−4622 (Vela Jr) supernova remnant

Published:2013-11-13 Issue:1 Volume:437 Page:976-993
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Obergaulinger M.,Iyudin A. F.,Müller E.,Smoot G. F.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/437/1/976/18465715/stt1966.pdf

Reference64 articles.

1. H.E.S.S. Observations of the Supernova Remnant RX J0852.0−4622: Shell‐Type Morphology and Spectrum of a Widely Extended Very High Energy Gamma‐Ray Source

2. Discovery of a young nearby supernova remnant

3. ChandraObservations of Galactic Supernova Remnant Vela Jr.: A New Sample of Thin Filaments Emitting Synchrotron X‐Rays

4. Nonthermal and thermal emission from the supernova remnant RX J1713.7-3946

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