Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds

We present results from the Austral Winter 2003 observing campaign of SPARO, a 450 micron polarimeter used with a two-meter telescope at South Pole. We mapped large-scale magnetic fields in four Giant Molecular Clouds (GMCs) in the Galactic disk: NGC 6334, the Carina Nebula, G333.6-0.2 and G331.5-0....

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Main Authors: Li, H., Griffin, G. S., Krejny, M., Novak, G., Loewenstein, R. F., Newcomb, M. G., Calisse, P. G., Chuss, D. T.
Format: Text
Language:unknown
Published: arXiv 2006
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Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0602455
https://arxiv.org/abs/astro-ph/0602455
id ftdatacite:10.48550/arxiv.astro-ph/0602455
record_format openpolar
spelling ftdatacite:10.48550/arxiv.astro-ph/0602455 2023-05-15T18:23:01+02:00 Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds Li, H. Griffin, G. S. Krejny, M. Novak, G. Loewenstein, R. F. Newcomb, M. G. Calisse, P. G. Chuss, D. T. 2006 https://dx.doi.org/10.48550/arxiv.astro-ph/0602455 https://arxiv.org/abs/astro-ph/0602455 unknown arXiv https://dx.doi.org/10.1086/505858 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2006 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0602455 https://doi.org/10.1086/505858 2022-04-01T15:57:26Z We present results from the Austral Winter 2003 observing campaign of SPARO, a 450 micron polarimeter used with a two-meter telescope at South Pole. We mapped large-scale magnetic fields in four Giant Molecular Clouds (GMCs) in the Galactic disk: NGC 6334, the Carina Nebula, G333.6-0.2 and G331.5-0.1. We find a statistically significant correlation of the inferred field directions with the orientation of the Galactic plane. Specifically, three of the four GMCs (NGC 6334 is the exception) have mean field directions that are within 15 degrees of the plane. The simplest interpretation is that the field direction tends to be preserved during the process of GMC formation. We have also carried out an analysis of published optical polarimetry data. For the closest of the SPARO GMCs, NGC 6334, we can compare the field direction in the cloud as measured by SPARO with the field direction in a larger region surrounding the cloud, as determined from optical polarimetry. For purposes of comparison, we also use optical polarimetry to determine field directions for other regions of similar size and distance. Overall, the results from this optical polarimetry analysis are consistent with our suggestion that field direction tends to be preserved during GMC formation. Finally, we compare the disorder in our magnetic field maps with the disorder seen in magnetic field maps derived from MHD turbulence simulations. We conclude from these comparisons that the magnetic energy density in our clouds is comparable to the turbulent energy density. : Submitted to Astrophys. J. (one color figure) Text South pole DataCite Metadata Store (German National Library of Science and Technology) Austral South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Li, H.
Griffin, G. S.
Krejny, M.
Novak, G.
Loewenstein, R. F.
Newcomb, M. G.
Calisse, P. G.
Chuss, D. T.
Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
topic_facet Astrophysics astro-ph
FOS Physical sciences
description We present results from the Austral Winter 2003 observing campaign of SPARO, a 450 micron polarimeter used with a two-meter telescope at South Pole. We mapped large-scale magnetic fields in four Giant Molecular Clouds (GMCs) in the Galactic disk: NGC 6334, the Carina Nebula, G333.6-0.2 and G331.5-0.1. We find a statistically significant correlation of the inferred field directions with the orientation of the Galactic plane. Specifically, three of the four GMCs (NGC 6334 is the exception) have mean field directions that are within 15 degrees of the plane. The simplest interpretation is that the field direction tends to be preserved during the process of GMC formation. We have also carried out an analysis of published optical polarimetry data. For the closest of the SPARO GMCs, NGC 6334, we can compare the field direction in the cloud as measured by SPARO with the field direction in a larger region surrounding the cloud, as determined from optical polarimetry. For purposes of comparison, we also use optical polarimetry to determine field directions for other regions of similar size and distance. Overall, the results from this optical polarimetry analysis are consistent with our suggestion that field direction tends to be preserved during GMC formation. Finally, we compare the disorder in our magnetic field maps with the disorder seen in magnetic field maps derived from MHD turbulence simulations. We conclude from these comparisons that the magnetic energy density in our clouds is comparable to the turbulent energy density. : Submitted to Astrophys. J. (one color figure)
format Text
author Li, H.
Griffin, G. S.
Krejny, M.
Novak, G.
Loewenstein, R. F.
Newcomb, M. G.
Calisse, P. G.
Chuss, D. T.
author_facet Li, H.
Griffin, G. S.
Krejny, M.
Novak, G.
Loewenstein, R. F.
Newcomb, M. G.
Calisse, P. G.
Chuss, D. T.
author_sort Li, H.
title Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
title_short Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
title_full Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
title_fullStr Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
title_full_unstemmed Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
title_sort results of sparo 2003: mapping magnetic fields in giant molecular clouds
publisher arXiv
publishDate 2006
url https://dx.doi.org/10.48550/arxiv.astro-ph/0602455
https://arxiv.org/abs/astro-ph/0602455
geographic Austral
South Pole
geographic_facet Austral
South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1086/505858
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0602455
https://doi.org/10.1086/505858
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