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 |
by | PERETTO 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. | |
o | Table 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 |
by | PERETTO 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. | |
o | Table 1, Fig.1: <[PAB2006] C-MMNN> (No. C-MM13) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |