Numerical simulations of supernova remnants in turbulent molecular clouds
Author:
Affiliation:
1. Department of Astronomy, University of Virginia, 530 McCormick Road, Charlottesville, VA 22904, USA
Funder
National Science Foundation
National Aeronautics and Space Administration
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/482/2/1602/26288903/sty2769.pdf
Reference138 articles.
1. Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT
2. OBSERVATION OF SUPERNOVA REMNANT IC 443 WITH THE FERMI LARGE AREA TELESCOPE
3. FERMILARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT W28 (G6.4–0.1)
4. Shocked Molecular Gas Associated with the Supernova Remnant W28
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