Dictionary of Nomenclature of Celestial Objects
(Last update: 17-Sep-2020)

Result of query: info cati SSY2008] IRAS HHMMm+DDMM MCS A$



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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 bySAITO 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. oTable 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 Originof the Acronym: S = Created by Simbad, the CDS Database

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