Details on Acronym: [WSL2017] | |
| [WSL2017] | (Watanabe+Sakai+Lopez-Sepulcre+, 2017)= ([WSL2017a]) |
| Write: | <<[WSL2017] CMM3A>> |
| N: | 8 |
| Object: | (smm) (SIMBAD class: smmRad = Sub-Millimetric Source) |
| Stat: | is completely incorporated in Simbad |
| Note: | ALMA Band 7 Cycle 2 observations of N=8 sources in the field of the NGC 2264 CMM3 core. |
| in source: | [PAB2006] C-MM3 |
| Ref: | =2017ApJ...847..108W |
| by | WATANABE Y. , SAKAI N., LOPEZ-SEPULCRE A., SAKAI T., HIROTA T., LIU S.-Y., SU Y.-N., YAMAMOTO S. |
| Astrophys. J., 847, 108-108 (2017) | |
| Discovery of striking difference of molecular-emission-line richness in the potential proto-binary system NGC 2264 CMM3. | |
| o | Table 1: <[WSL2017] CMM3A> (Nos A-H). |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [WSL2017a] | |
| [WSL2017a] | (Watanabe+Sakai+Lopez-Sepulcre+, 2017) |
| ***** | Avoid the usage of [WSL2017a], prefer [WSL2017] |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |