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A Molecular Filament Threaded by Helical Magnetic Fields?

Authors :
Pierre Hily-Blant
Edith Falgarone
G. Pineau des Forêts
Thomas G. Phillips
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA)
École normale supérieure - Paris (ENS-PSL)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP)
Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS)
Institut d'astrophysique spatiale (IAS)
Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES)
Cahill Center for Astronomy and Astrophysics, California Institute of Technology
Source :
Astrophysics and Space Science, Astrophysics and Space Science, 2004, 292, pp.285-289. ⟨10.1023/B:ASTR.0000045029.17637.3b⟩
Publication Year :
2004
Publisher :
Springer Science and Business Media LLC, 2004.

Abstract

International audience; 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 n H 2= 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.

Details

ISSN :
0004640X and 1572946X
Volume :
292
Database :
OpenAIRE
Journal :
Astrophysics and Space Science
Accession number :
edsair.doi.dedup.....4b58812d3886122adda177b08d6eb44a
Full Text :
https://doi.org/10.1023/b:astr.0000045029.17637.3b