Details on Acronym: [KRR2001] | |
| [KRR2001] | (Koo+Rho+Reach+, 2001) |
| Write: | <<[KRR2001] Cloud W>> <<[KRR2001] Cloud WW>> <<[KRR2001] Cloud WWN>> <<[KRR2001] HB 21 BML WN>> |
| N: | 3+1+4+4+5 |
| Object: | Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud) |
| Stat: | is completely incorporated in Simbad |
| Note: | Study of the SNR HBH 21. N=4 CO clouds (Nos N, S, E, NW). Cloud NW has 4 components NW1 to NW4. N=4 emission clouds in the Center (Nos C1-C2) and in the North (Nos N3-N4). N=5 peak positions or clumps in Cloud N and S, in the format BML stands for Broad Molecular Line. |
| in source: | HBH 21 |
| Ref: | =2001ApJ...552..175K |
| by | KOO B.-C. , RHO J., REACH W.T., JUNG J., MANGUM J.G. |
| Astrophys. J., 552, 175-188 (2001) | |
| Shocked molecular gas in the supernova remnant HB 21. | |
| o | Fig.2, Table 3: Cloud A, B, C = [TFL90] A, B, C. |
| o | Fig.2: <[KRR2001] Cloud W> (Nos N, S). Table 1: <[KRR2001] HB 21 BML WN> (Nos N1-N2, S1-S3). |
| Ref: | =2006ApJ...637..283B |
| by | BYUN D.-Y. , KOO B.-C., TATEMATSU K., SUNADA K. |
| Astrophys. J., 637, 283-295 (2006) | |
| Interaction between the supernova remnant HB 21 and molecular clouds. | |
| o | Fig. 1: <[KRR2001] Cloud WW> (Nos E, NW) added. Fig. 3: <[KRR2001] Cloud WWN> (Nos NW1-NW4). Table 2, Fig. 5: <[KRR2001] Cloud WN> (Nos C1-C2, N3-N4). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |