Details on Acronym: [MKW2020] | |
| [MKW2020] | (McLeod+Kruijssen+Weisz+, 2020) |
| Write: | <<[MKW2020] 11N-N>> <<[MKW2020] 11N-WRN>> |
| N: | 13+4 |
| Object: | 0 * + WR (SIMBAD class: Star) |
| Stat: | is completely incorporated in Simbad |
| Note: | VLT MUSE observations of N=4+9 O-type stars and N=2+2 Wolf-Rayet stars in the HII region complexes [DCL88] 118 and [DCL88] 119 respectively. |
| in source: | [DCL88] 118 |
| in source: | [DCL88] 119 |
| Ref: | =2020ApJ...891...25M |
| by | McLEOD A.F. , KRUIJSSEN J.M.D., WEISZ D.R., ZEIDLER P., SCHRUBA A., DALCANTON J.J., LONGMORE S.N., CHEVANCE M., FAESI C.M., BYLER N. |
| Astrophys. J., 891, 25-25 (2020) | |
| Stellar feedback and resolved stellar IFU spectroscopy in the nearby spiral galaxy NGC 300. | |
| o | Fig. 5, Table 3: <[MKW2020] 11N-N> (Nos 118-1 to 118-4, 119-1 to 119-9). Fig. 5, Table 4: <[MKW2020] 11N-WRN> (Nos 118-WR1 to 118-WR2, 119-WR1 to 119-WR2). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |