The Intrinsic Shapes of Molecular Cloud Fragments over a Range of Length Scales
Author(s) -
C. E. Jones,
Sarbani Basu
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/339230
Subject(s) - prolate spheroid , oblate spheroid , molecular cloud , range (aeronautics) , physics , astrophysics , materials science , classical mechanics , stars , composite material
We decipher intrinsic three-dimensional shape distributions of molecularclouds, cloud cores, Bok globules, and condensations using recently compiledcatalogues of observed axis ratios for these objects mapped in carbon monoxide,ammonia, through optical selection, or in continuum dust emission. We applystatistical techniques to compare assumed intrinsic axis ratio distributionswith observed projected axis ratio distributions. Intrinsically triaxial shapesproduce projected distributions which agree with observations. Molecular cloudsmapped in $^{12}$CO are intrinsically triaxial but more nearly prolate thanoblate, while the smaller cloud cores, Bok globules, and condensations are alsointrinsically triaxial but more nearly oblate than prolate.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom