A Molecular Filament Threaded by Helical Magnetic Fields?

被引:0
|
作者
P. Hily-Blant
E. Falgarone
G. Pineau des Forêts
T. G. Phillips
机构
[1] LRA/LERMA,
[2] Ecole Normale Supérieure,undefined
[3] Institut d'Astrophysique Spatiale,undefined
[4] California Institute of Technology,undefined
来源
Astrophysics and Space Science | 2004年 / 292卷
关键词
molecular clouds; dense core; magnetic fields;
D O I
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中图分类号
学科分类号
摘要
We present a multitransition study in the 13CO(1-0), 12CO(2-1), 12CO(3-2) and 12CO(4-3) lines of a parsec scale elongated structure connected to a low-mass dense core. Densities larger than nH2 = 104 cm−3 are inferred in the central regions of this structure, supporting the proposition that it is a genuine filament denser than its environment. The sharp observed drop of the 12CO and 13CO emissions requires a power law density fall-off steeper than r−1 although a single density law cannot reproduce the spatial shift of 0.1 pc between the 13CO and 12CO drops. Our results support the previous proposition that this elongated structure is a filament threaded by helical magnetic fields, channeling the gas inflow onto the dense core.
引用
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页码:285 / 289
页数:4
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