The SNR G160.9+2.6 blast wave interaction with the star forming region Sh-219

As core collapse supernovae often occur close to their parent molecular clouds,it is expected that interactions between core collapse supernova remnants (SNRs)and young stellar objects (YSOs) forming in those clouds are common. To date virgul40SNRmolecular cloud associations have been confirmed. SNR shock waves impact theevolution of local YSOs which has implications for star/planet formation. It isimportant to correctly map the progression of an SNR blast wave through astarforming region (SFR), assess the impact of the SNR on the SFR, and viceversa. We aim to perform such a study for the case of the SNR G160.9+2.6interaction with Sh219. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]