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Query : 2011A&A...530A.101M |
2011A&A...530A.101M - Astronomy and Astrophysics, volume 530A, 101-101 (2011/6-1)
Accuracy of core mass estimates in simulated observations of dust emission.
MALINEN J., JUVELA M., COLLINS D.C., LUNTTILA T. and PADOAN P.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): ISM: structure - ISM: clouds - stars: formation - radiative transfer - magnetohydrodynamics (MHD) - submillimeter: ISM
Simbad objects: 1
Number of rows : 1 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
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1 | IC 5146 | OpC | 21 53 29.3 | +47 14 46 | ~ | 467 | 2 |
Query : 2011A&A...530A.101M |
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Hierarchy :
number of linked objects
whatever the membership probability is (see description here ) :
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information for this acronym in the dictionary of nomenclature.
Identifiers (12) :
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IC 5146 | LBN 424 | NAME Cocoon Nebula | OCl 213.0 |
C 2151+470 | LBN 094.43-05.58 | OCISM 43 | [KC2019] Theia 88 |
Cl Collinder 470 | Min 2-70 | OCl 213 | [KPS2012] MWSC 3571 |
References (467 between 1850 and 2024) (Total 467)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system). Follow new references on this object |
Observing logs
Data at NED - NASA/IPAC Extragalactic Database : IC 5146
Search by coordinates in Vizier (radius: 5 arcsec)
Indications mainly about references on other documents
Notes (1) :
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``the IC makes no mention of a star cluster here, and neither do the discoverersof the IC 5146 nebula (the "Cocoon Nebula"), Espin (1900) and Wolf (1904).Collinder appears to have been the first to identify a star cluster here(even though he also used the IC 5146 name incorrectly), so the preferred namewould seem to be Collinder 470. Details of this are given in Brent A. Archinaland Steven's Hynes book "Star Clusters", pp. 127-128.''
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