Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati PAB2006] D-MMNN$
.

Details on Acronym:   [PAB2006]
  
[PAB2006] (Peretto+Andre+Belloche, 2006)
Write:<<[PAB2006] C-MMNN>>
<<[PAB2006] D-MMNN>>
N: 13+15
Object:(mm)  (SIMBAD class: mmRad = 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