Details on Acronym: [KRE2018] | |
| [KRE2018] | (Kalari+Rubio+Elmegreen+, 2018) |
| Write: | <<[KRE2018] KNN>> <<[KRE2018] KNN-A>> |
| N: | 3+3 |
| Object: | MCld + Poss. YSO (SIMBAD class: Unknown = Object of Unknown Nature) |
| Stat: | is completely incorporated in Simbad |
| Note: | SEST CO(2-1) and VLT ISAAC observations of N=3 CO molecular clouds and N=3 candidate YSOs towards the young stellar cluster RMC 136 in 30 Doradus. In the format, KN stands for "knot", as the clouds form a chain separated in velocity. Use of archival Spitzer SAGE and HERITAGE data. |
| in source: | Magellanic Clouds:LMC:30 Dor Nebula = 30 Dor Nebula |
| in source: | Magellanic Clouds:LMC:RMC 136 = RMC 136 |
| Ref: | =2018ApJ...852...71K |
| by | KALARI V.M. , RUBIO M., ELMEGREEN B.G., GUZMAN V.V., ZINNECKER H., HERRERA C.N. |
| Astrophys. J., 852, 71-71 (2018) | |
| Pillars of creation among destruction: star formation in molecular clouds near R136 in 30 Doradus. | |
| o | Fig. 2, Table 1: <[KRE2018] KNN> (Nos KN1-KN3). Fig. 6, Table 2: <[KRE2018] KNN-A> (Nos KN2-A to KN2-B, KN3-A). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |