Observations and Analysis of High-Resolution Magnetic Field Structures in Molecular Clouds
hal.structure.identifier | AMOR 2012 | |
dc.contributor.author | TANG, Ya-Wen | |
dc.contributor.author | KOCH, Patrick M. | |
dc.contributor.author | HO, Paul T. P. | |
dc.date.created | 2012-02-21 | |
dc.description.abstractEn | Recent high-angular-resolution (up to 0.7") dust polarization observations toward star forming regions are summarized. With the Sub-Millimeter Array, the emission from the dense structures is traced and resolved. The detected magnetic field morphologies vary from hourglass-like structures to isolated patches depending on the evolutionary stage of the source. These observed features have also served as a testbed to develop new analysis methods, with a particular focus on quantifying the role of the magnetic field in the star formation process. | |
dc.language.iso | en | |
dc.subject.en | Astrophysics | |
dc.subject.en | Galaxy Astrophysics | |
dc.title.en | Observations and Analysis of High-Resolution Magnetic Field Structures in Molecular Clouds | |
dc.type | Document de travail - Pré-publication | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.identifier.arxiv | 1202.4635 | |
hal.identifier | hal-00674423 | |
hal.version | 1 | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00674423v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=TANG,%20Ya-Wen&KOCH,%20Patrick%20M.&HO,%20Paul%20T.%20P.&rft.genre=preprint |
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