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ALMA reveals the co...
ALMA reveals the coherence of the magnetic field geometry in OH 231.8+4.2
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- Sabin, L. (författare)
- Universidad Nacional Autónoma de México (UNAM),Universidad Nacional Autonoma de Mexico
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- Sahai, R. (författare)
- California Institute of Technology (Caltech)
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- Vlemmings, Wouter, 1974 (författare)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Zhang, Q. (författare)
- Harvard-Smithsonian Center for Astrophysics
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- Zijlstra, A. A. (författare)
- University of Manchester
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- Gledhill, T. (författare)
- University of Hertfordshire
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- Huarte-Espinosa, M. (författare)
- University of Houston
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- Sanchez, A. F. Perez (författare)
- European Southern Observatory Santiago,Universiteit Leiden (UL),Leiden University (UL)
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- Lagadec, E. (författare)
- Observatoire de la Cote d'Azur
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- Navarro, S. G. (författare)
- Universidad de Guadalajara,University of Guadalajara
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(creator_code:org_t)
- 2020-05-23
- 2020
- Engelska.
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Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 495:4, s. 4297-4305
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- In a continuing effort to investigate the role of magnetic fields in evolved low- and intermediate-mass stars (principally regarding the shaping of their envelopes), we present new Atacama Large Millimeter/submillimeter Array (ALMA) high-resolution polarization data obtained for the nebula OH 231.8+4.2. We found that the polarized emission likely arises from aligned grains in the presence of magnetic fields rather than radiative alignment and self-scattering. The ALMA data show well organized electric field orientations in most of the nebula and the inferred magnetic field vectors (rotated by 90 degrees) trace an hourglass morphology centred on the central system of the nebula. One region in the southern part of OH 231.8+4.2 shows a less organized distribution probably due to the shocked environment. These findings, in conjunction with earlier investigations (maser studies and dust emission analysis at other scales and wavelengths) suggest an overall magnetic hourglass located inside a toroidal field. We propose the idea that the magnetic field structure is closely related to the architecture of a magnetic tower and that the outflows were therefore magnetically launched. While the current dynamical effect of the fields might be weak in the equatorial plane principally due to the evolution of the envelope, it would still be affecting the outflows. In that regard, the measurement of the magnetic field at the stellar surface, which is still missing, combined with a full magnetohydrodynamic treatment are required to better understand and constrain the events occurring in OH 231.8+4.2.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
- NATURVETENSKAP -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
- NATURVETENSKAP -- Fysik -- Den kondenserade materiens fysik (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Condensed Matter Physics (hsv//eng)
Nyckelord
- stars: AGB and post-AGB
- magnetic fields
- polarization
- ISM: individual objects: OH231.8+4.2
- ISM: jets and outflows
Publikations- och innehållstyp
- art (ämneskategori)
- ref (ämneskategori)
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Sabin, L.
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Sahai, R.
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Vlemmings, Woute ...
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Zhang, Q.
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Zijlstra, A. A.
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Gledhill, T.
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visa fler...
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Huarte-Espinosa, ...
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Sanchez, A. F. P ...
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Lagadec, E.
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Navarro, S. G.
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visa färre...
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