Details on Acronym: S | |
| S | (Searle) |
| ***** | Avoid the usage of S, prefer [S71] |
| Origin | of the Acronym: L (1996MNRAS.283..990T) |
Details on Acronym: [S71] | |
| [S71] | (Searle, 1971)= (S) = [S71a] = (Searle) |
| Write: | <<[S71] M 33 NN>> <<[S71] M 51 N>> <<[S71] M 101 NN>> |
| N: | 30+5+13 |
| Object: | Region (SIMBAD class: PartofG = Part of a Galaxy) |
| Note: | Table 2: 'M 33 NN', N=30 'M 51 N', N=5 'M 101 NN', N=13 |
| in source: | M 33 = NGC 598 |
| in source: | M 51 = NGC 5194 |
| in source: | M 101 = NGC 5457 |
| Ref: | =1971ApJ...168..327S |
| by | SEARLE L. |
| Astrophys. J., 168, 327-341 (1971) | |
| Evidence for composition gradients across the disks of spiral galaxies. | |
| o | Table 2: <[S71] M 33 NN> N=30, Table 2: <[S71] M 101 NN> N=13, <[S71] M 51 N> N=5 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [S71a] | |
| [S71a] | (Searle, 1971) |
| ***** | Avoid the usage of [S71a], prefer [S71] |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: Searle | |
| Searle | (Searle) |
| ***** | Avoid the usage of Searle, prefer [S71] |
| Origin | of the Acronym: L (1975ApJ...199..591S) |