Multi-Scale Analysis of Magnetic Fields in and around OMC-1, OMC-2, and OMC-3

Bibcode
2011ASPC..449..105P
Poidevin, F.; Bastien, P.; Jones, T. J.; Matthews, B. C.
Referencia bibliográfica

Astronomical Polarimetry 2008: Science from Small to Large Telescopes. Proceedings of a Workshop held at Fairmont Le Manoir Richelieu, La Malbaie, Quebec, Canada 6-11 July 2008. Edited by Pierre Bastien, Nadine Manset, Dan P. Clemens, and Nicole St-Louis. ASP Conference Series, Vol. 449. San Francisco: Astronomical Society of the Pacific, 2012., p.105

Fecha de publicación:
11
2011
Número de autores
4
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
Comparisons of visible/NIR and FIR/submm data are investigated on several spatial scales in and around the OMC-1, OMC-2 and OMC-3 star-forming regions in Orion A. Our conclusions are that the magnetic field orientations observed in the filaments are smoothly consistent with the ones probed around OMC-1, OMC-2 and OMC-3. Analysis of NIR and submm polarimetry around the BN object suggests that a rotation of the magnetic field orientation by ≍ 40° could exist along lines-of-sight in this region of the galaxy.
Tipo
Sin árbitro

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