2002ApJ...569..280J


Query : 2002ApJ...569..280J

2002ApJ...569..280J - Astrophys. J., 569, 280-287 (2002/April-2)

The intrinsic shapes of molecular cloud fragments over a range of length scales.

JONES C.E. and BASU S.

Abstract (from CDS):

We decipher intrinsic three-dimensional shape distributions of molecular clouds, cloud cores, Bok globules, and condensations using recently compiled catalogs of observed axis ratios for these objects mapped in carbon monoxide, in ammonia, through optical selection, or in continuum dust emission. We apply statistical techniques to compare assumed intrinsic axis ratio distributions with observed projected axis ratio distributions. Intrinsically triaxial shapes produce projected distributions that agree with observations. Molecular clouds mapped in 12CO are intrinsically triaxial but more nearly prolate than oblate, while the smaller cloud cores, Bok globules, and condensations are also intrinsically triaxial but more nearly oblate than prolate.

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Journal keyword(s): ISM: Clouds - ISM: Globules - ISM: Structure - Stars: Formation

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Flame Nebula HII 05 41 42.7 -01 54 44           ~ 715 1
2 NAME Ori B MoC 05 41 43.0 -01 54 44           ~ 1498 0
3 M 78 RNe 05 46 45.8 +00 04 45   8.0       ~ 397 0
4 NGC 2071 RNe 05 47 10 +00 18.0           ~ 661 1

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