Dictionary of Nomenclature of Celestial Objects
(Last update: 02-Nov-2023)

Result of query: info cati PAB2006] C-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