Probing magnetohydrodynamic shocks with high-J CO observations: W28F

Author: Gusdorf A.   Anderl S.   Güsten R.   Stutzki J.   Hübers H.-W.   Hartogh P.   Heyminck S.   Okada Y.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|542|issue|L19-L19

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.542, Iss.issue, 2012-05, pp. : L19-L19

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Abstract

Context. Observing supernova remnants (SNRs) and modelling the shocks they are associated with is the best way to quantify the energy SNRs re-distribute back into the interstellar medium (ISM).