Details on Acronym: GMA | |
| GMA | (Giant Molecular Assoc.) |
| ***** | Avoid the usage of GMA, prefer [TM97] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [TM97] | |
| [TM97] | (Thornley+Mundy, 1997)= (GMA) |
| Write: | <<[TM97] NGC 5055 NN>> <<[TM97] NGC 4414 NN>> |
| N: | 17+13 |
| Object: | Giant Molecular Assoc. (SIMBAD class: PartofG = Part of a Galaxy) |
| Stat: | is completely incorporated in Simbad |
| in source: | NGC 5055 |
| in source: | NGC 4414 |
| Ref: | =1997ApJ...484..202T |
| by | THORNLEY M.D. , MUNDY L.G. |
| Astrophys. J., 484, 202-221 (1997) | |
| Are flocculent spirals devoid of density waves? gas morphology and kinematics in NGC 5055. | |
| o | Table 3: <[TM97] NGC 5055 NN> (Nos 1-17) |
| Ref: | =1997ApJ...490..682T |
| by | THORNLEY M.D. , MUNDY L.G. |
| Astrophys. J., 490, 682-697 (1997) | |
| Dynamic and stochastic influences on spiral structure in the flocculent spiral NGC 4414. | |
| o | Table 2: <[TM97] NGC 4414 NN> (Nos 1-13) |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |