| -Apr-2022 - AE - Modification (%s added) | Details on Acronym: [ITL2019] | |
| [ITL2019] | ||
| Write: | <<[ITL2019] RN>> <<[ITL2019] SMAN>> <<[ITL2019] CNN>> | |
| N: | 2+3+12 | |
| Object: | (Rad) + mm core + Clump (SIMBAD class: Unknown = Object of Unknown Nature) | |
| Stat: | is completely incorporated in Simbad | |
| Note: | GMRT (610 and 1390MHz), SMA (1.1mm), and UKIRT (NIR) observations of N=2 radio components, N=3 millimeter cores, and N=12 clumps in the field of EGO G012.42+0.50. | |
| Ref: | =2019MNRAS.485.1775I | |
| by | ISSAC N. , TEJ A., LIU T., VARRICATT W., VIG S., ISHWARA CHANDRA C.H., SCHULTHEIS M. | |
| Mon. Not. R. Astron. Soc., 485, 1775-1799 (2019) | ||
| Initial phases of high-mass star formation: a multiwavelength study towards the extended green object G12.42+0.50. | ||
| o | Fig. 2, Table 4: <[ITL2019] RN> (Nos R1-R2). Fig. 7, Table 6: <[ITL2019] SMAN> (Nos SMA1-SMA3). Fig. 9, Table 8: <[ITL2019] CNN> (Nos C1-C12). | |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database | |