Details on Acronym: [KVS2019] | |
| [KVS2019] | (Kavanagh+Vink+Sasaki+, 2019) |
| Write: | <<[KVS2019] NN>> |
| N: | 10 |
| Object: | (X) (SIMBAD class: X = X-ray Source) |
| Note: | Chandra observations of N=10 X-ray sources around 30 Dor C in the LMC. |
| in source: | Magellanic Clouds:LMC:30 Dor C = 30 Dor C |
| Ref: | =2019A&A...621A.138K |
| by | KAVANAGH P.J. , VINK J., SASAKI M., CHU Y.-H., FILIPOVIC M.D., OHM S., HABERL F., MANOJLOVIC P., MAGGI P. |
| Astron. Astrophys., 621A, 138-138 (2019) | |
| Magnetic field estimates from the X-ray synchrotron emitting rims of the 30 Dor C superbubble and the implications for the nature of 30 Dor C's TeV emission. | |
| o | Table 1: <[KVS2019] NN> (Nos 1-10). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |