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Magnetically Dominated Strands of Cold Hydrogen in the Riegel-Crutcher Cloud

Citation

McClure-Griffiths, NM and Dickey, JM and Gaensler, BM and Green, AJ and Haverkorn, M, Magnetically Dominated Strands of Cold Hydrogen in the Riegel-Crutcher Cloud, The Astrophysical Journal, 652, (2) pp. 1339-1347. ISSN 0004-637X (2006) [Refereed Article]

DOI: doi:10.1086/508706

Abstract

We present new high-resolution (100″) neutral hydrogen (H I) self-absorption images of the Riegel-Crutcher cloud obtained with the Australia Telescope Compact Array and the Parkes Radio Telescope. The Riegel-Crutcher cloud lies in the direction of the Galactic center at a distance of 125 ± 25 pc. Our observations resolve the very large, nearby sheet of cold hydrogen into a spectacular network of dozens of hairlike filaments. Individual filaments are remarkably elongated, being up to 17 pc long with widths of less than ∼0.1 pc. The strands are reasonably cold, with spin temperatures of ∼40 K and in many places appearing to have optical depths larger than 1. Comparing the H I images with observations of stellar polarization, we show that the filaments are very well aligned with the ambient magnetic field. We argue that the structure of the cloud has been determined by its magnetic field. In order for the cloud to be magnetically dominated the magnetic field strength must be >30 μG. © 2006. The American Astronomical Society. All rights reserved.

Item Details

Item Type:Refereed Article
Research Division:Physical Sciences
Research Group:Astronomical and Space Sciences
Research Field:Galactic Astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Physical Sciences
Author:Dickey, JM (Professor John Dickey)
ID Code:41056
Year Published:2006
Web of Science® Times Cited:38
Deposited By:Physics
Deposited On:2006-08-01
Last Modified:2007-03-21
Downloads:0

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