Dictionary of Nomenclature of Celestial Objects

 2011] (Not yet in Simbad)
 Write:<< KN>>  
<< ICNN>>
<< GLL.ll+B.bb>> Object:smm Clump  (SIMBAD class: Radio(sub-mm) = sub-millimetric source) in source:PN K 3-50 in source:IC 5146 Ref:=2011ApJ...730..142R byROY A. , ADE P.A.R., BOCK J.J., BRUNT C.M., CHAPIN E.L., DEVLIN M.J., DICKER S.R., FRANCE K., GIBB A.G., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V. Astrophys. J., 730, 142 (2011) Deconvolution of images from BLAST 2005: insight into the K3-50 and IC 5146 star-forming regions. oTable 1, col(1): <[RAB2011] KN> (Nos K1-K5) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=5. Table 2, col(1): <[RAB2011] ICNN> (Nos IC1-IC10) = Table 2, col(2): <BLAST JHHMMSS+DDMMSS> N=10. Fig. 10: <[RAB2011] GLL.ll+B.bb> N=3. Originof the Acronym: S = Created by Simbad, the CDS Database
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