Details on Acronym: [SSY2008] | |
| [SSY2008] | (Saito+Saito+Yonekura+, 2008) |
| Write: | <<[SSY2008] IRAS HHMMm+DDMM Core A>> <<[SSY2008] IRAS HHMMm+DDMM Core AA>> <<[SSY2008] IRAS HHMMm+DDMM MCS A>> |
| N: | 177+13 |
| Object: | C18O Core + mm Continuum Source (SIMBAD class: MolCld = Molecular Cloud) |
| Note: | C18O(1-0) observations with the Nobeyama Millimeter Array toward dense clumps in N=6 IRAS star-forming regions. N=177 cores associated with N=13 Millimeter Continuum Sources (MCS) are found. |
| in source: | IRAS 05375+3540 |
| in source: | IRAS 06056+2131 |
| in source: | IRAS 06061+2151 |
| in source: | IRAS 06117+1350 |
| in source: | IRAS 19442+2427 |
| in source: | IRAS 19446+2505 |
| Ref: | =2008ApJS..178..302S |
| by | SAITO H. , SAITO M., YONEKURA Y., NAKAMURA F. |
| Astrophys. J., Suppl. Ser., 178, 302-329 (2008) | |
| High-resolution studies of the multiple-core systems toward cluster-forming regions including massive stars. | |
| o | Table 3: <[SSY2008] IRAS HHMMm+DDMM Core A>, <[SSY2008] IRAS HHMMm+DDMM Core AA>, N=21+19+24+28+38+41. Table 5: <[SSY2008] IRAS HHMMm+DDMM MCS A> N=2+2+2+1+3+3. |
| =E= | Catalogue in electronic form as J/ApJS/178/302 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |