Shocked molecular gas in the supernova remnant HB 21

We have carried out (CO)-C-12 J = 2-1 line observations of the supernova re mnant (SNR) HE 21 in order to search for evidence of interaction with molec ular clouds. We mapped the eastern half (80' x 110') of the SNR almost comp letely. Molecular gas appears to be distributed mainly along the boundary o f the SNR, but the overall distribution has little correlation either with the distortion of the SNR boundary or with the distribution of radio bright ness. Along the eastern boundary, where the SNR was considered to be intera cting with molecular clouds in previous studies, we have not found any stro ng evidence for the interaction. Instead, we detected broad (20-40 km s(-1) ) CO emission lines in the northern and southern parts of the SNR. In the n orthern area, the broad-line emitting cloud is composed of a small (similar to2' or 0.5 pc), very bright, U-shaped part and several clumps scattered a round it. There is a significant enhancement of radio emission with a flat (-0.28 +/- 0.17) spectral index possibly associated with this cloud. In the southern area, the broad-line emitting cloud is filamentary and appears to form an elongated loop of similar to 30' in extent. Small (less than or si milar to 1.'2 or 0.3 pc), bright clumps are seen along the filamentary stru cture. We have obtained sensitive J = 1-0 and J = 2-1 spectra of (CO)-C-12 and (CO)-C-13 molecules toward several peak positions. The intensity of (CO )-C-12 J = 2-1 emission is low (T-mb < 7 K) and the ratio of (CO)-C-12 J = 2-1 to J = 1-0 integrated intensities is high (1.6-2.3), which suggests tha t the emission is from warm, dense, and clumpy gas. We have applied a large velocity gradient analysis to derive their physical parameters. The detect ed broad CO lines are believed to be emitted from the fast-moving molecular gas swept up by the SNR shock. The small (<less than or similar to>20 km s (-1)) shock velocity suggests that the shock is a nondissociating C-shock. We discuss the correlation of the shocked molecular gas with the previously detected, shocked atomic gas and the associated infrared emission.