.
.
Details on Acronym: [KJD2006]
[KJD2006] (Kirk+Johnstone+Di Francesco, 2006)= (SMM) Write:<<[KJD2006] SMM JHHMMmm+DDMMm>>
<<[KJD2006] EC NN>>
<<[KJD2006] ESC NN>> N: 58+39+11 Object:(smm) + Core (SIMBAD class: PartofCloud = Part of Cloud) Stat:is completely incorporated in Simbad Note:JCMT SCUBA observations of the Perseus Molecular Cloud.
N=58 sub-mm clumps (SMM in the format) + N=39 Extinction Core (EC in the format) + N=11 Extinction Super Cores (ESC in the format).
See also Paper II: [KJT2007]. in source:NAME Perseus Molecular Cloud Ref:=2006ApJ...646.1009K byKIRK H. , JOHNSTONE D., DI FRANCESCO J. Astrophys. J., 646, 1009-1023 (2006) The large- and small-scale structures of dust in the star-forming Perseus molecular cloud. o(Erratum) erratum vol. 669, p. 657 (2007) oTable 1: <[KJD2006] SMM JHHMMmm+DDMMm> N=58. Table 2: <[KJD2006] EC NN> (Nos 1-39). Table 3: <[KJD2006] ESC NN> (Nos 1-11). =E=Catalogue in electronic form as J/ApJ/646/1009 Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym: SMM
SMM (SubMilliMeter source) ***** Avoid the usage of SMM, prefer [KJD2006] Originof the Acronym: A = Assigned by the author(s)
© Université de Strasbourg/CNRS
• Contact