Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Oct-2021)

Result of query: info cati PAB2006]$

Details on Acronym:   [PAB2006]
   [PAB2006] (Peretto+Andre+Belloche, 2006) Write:<<[PAB2006] C-MMNN>>
<<[PAB2006] D-MMNN>> N: 13+15 Object:(mm)  (SIMBAD class: Radio(mm) = millimetric Radio-source) Stat:is completely incorporated in Simbad Note:MAMBO bolometer array and HERA heterodyne array on the IRAM 30m telescope observations of NGC 2264.
Two parts of NGC 2264 are studied: NGC 2264C and D.
See also [TLY2006]. in source:NGC 2264 Ref:=2006A&A...445..979P byPERETTO N. , ANDRE P., BELLOCHE A. Astron. Astrophys., 445, 979-998 (2006) Probing the formation of intermediate- to high-mass stars in protoclusters. A detailed millimeter study of the NGC 2264 clumps. oTable 1, Figs 2, 3: <[PAB2006] C-MMNN> (Nos C-MM01 to C-MM12), <[PAB2006] D-MMNN> (Nos D-MM01 to D-MM15). Ref:=2007A&A...464..983P byPERETTO N. , HENNEBELLE P., ANDRE P. Astron. Astrophys., 464, 983-994 (2007) Probing the formation of intermediate- to high-mass stars in protoclusters. II. Comparison between millimeter interferometric observations of NGC 2264-C and SPH simulations of a collapsing clump. oTable 1, Fig.1: <[PAB2006] C-MMNN> (No. C-MM13) added. Originof the Acronym: S = Created by Simbad, the CDS Database

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