Details on Acronym: [FCC2002] | |
| [FCC2002] | (Furuya+Cesaroni+Codella+, 2002) |
| Write: | <<[FCC2002] ANa>> |
| N: | 4+2+3 |
| Object: | * (SIMBAD class: YSO = Young Stellar Object) |
| Stat: | is completely incorporated in Simbad |
| Note: | N=4 stars in the field of the star-forming region GAL 024.78+00.08. 2004ApJ...601L.187B: Star A is resolved in two separate cores. 2011A&A...532A..91B: Cores A1 and A2 are resolved into three and two cores respectively. |
| Ref: | =2002A&A...390L...1F |
| by | FURUYA R.S. , CESARONI R., CODELLA C., TESTI L., BACHILLER R., TAFALLA M. |
| Astron. Astrophys., 390, 1-4 (2002) | |
| G24.78+0.08: A cluster of high-mass (proto)stars. | |
| o | Fig.1, Table 1: <[FCC2002] A> (Nos A-D). |
| Ref: | =2004ApJ...601L.187B |
| by | BELTRAN M.T. , CESARONI R., NERI R., CODELLA C., FURUYA R.S., TESTI L., OLMI L. |
| Astrophys. J., 601, 187-190 (2004) | |
| Rotating disks in high-mass young stellar objects. | |
| o | Fig.1: <[FCC2002] AN> (Nos A1-A2) added. |
| Ref: | =2011A&A...532A..91B |
| by | BELTRAN M.T. , CESARONI R., ZHANG Q., GALVAN-MADRID R., BEUTHER H., FALLSCHEER C., NERI R., CODELLA C. |
| Astron. Astrophys., 532A, 91-91 (2011) | |
| Molecular outflows and hot molecular cores in G24.78+0.08 at sub-arcsecond angular resolution. | |
| o | Fig. 1, Table 2: <[FCC2002] ANa> (Nos A1b-A1c, A2b) added. |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |