Details on Acronym: [BEP2016] | |
[BEP2016] | (Busquet+Estalella+Palau+, 2016) |
Write: | <<[BEP2016] Hub-W MMNa>> |
N: | 9+17 |
Object: | (mm) (SIMBAD class: mmRad = Millimetric Radio Source) |
Stat: | is completely incorporated in Simbad |
Note: | SMA 1.3mm continuum observations of N=9+17 submillimeter sources toward the two hubs of the IR dark cloud G014.225-0.506. |
in source: | M 17:NAME M17 SWex = NAME M17 SWex |
Ref: | =2016ApJ...819..139B |
by | BUSQUET G. , ESTALELLA R., PALAU A., LIU H.B., ZHANG Q., GIRART J.M., DE GREGORIO-MONSALVO I., PILLAI T., ANGLADA G., HO P.T.P. |
Astrophys. J., 819, 139 (2016) | |
What is controlling the fragmentation in the infrared dark cloud G14.225-0.506?: different levels of fragmentation in twin hubs. | |
o | Table 4: <[BEP2016] Hub-N MMNa> N=9 (Nos MM1a-MM1g, MM2, MM3), <[BEP2016] Hub-S MMa> N=17 (Nos MM1a to MM9). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |