Details on Acronym: BML | |
| BML | (Broad Molecular Line) |
| ***** | Avoid the usage of BML, prefer [RRJ2005] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [RRJ2005] | |
| [RRJ2005] | (Reach+Rho+Jarrett, 2005)= (BML) |
| Write: | <<[RRJ2005] W28 BML N>> |
| N: | 5 |
| Object: | Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud) |
| Stat: | is completely incorporated in Simbad |
| Note: | High-resolution mm-wave and NIR observations of the SNR W 28. N=5 BML (Broad Molecular Line) regions in W 28. |
| in source: | W 28 |
| Ref: | =2005ApJ...618..297R |
| by | REACH W.T. , RHO J., JARRETT T.H. |
| Astrophys. J., 618, 297-320 (2005) | |
| Shocked molecular gas in the supernova remnants W28 and W44: near-infrared and millimeter-wave observations. | |
| o | Table 2, Fig.13: <[RRJ2005] W28 BML N> (Nos 1-5). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |