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Recolector de Ciencia Abierta, RECOLECTA
Conference object . 2020
Full-Text: http://dx.doi.org/10.1017/S1743921317010092
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Proceedings of the International Astronomical Union
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Magnetic fields and radio emission processes in maser-emitting planetary nebulae

descriptionPublicationkeyboard_double_arrow_right Article , Conference object , Other literature type 01 Sep 2017 Spain English Publisher:Cambridge University Press (CUP)Journal:Proceedings of the International Astronomical Union, volume 13, pages 397-398 (issn: 1743-9213, eissn: 1743-9221, Copyright policy )
Authors: Uscanga, L.; Gómez, José F.; Green, J.A.; Suárez, O.; Qiao, H. -H.; Walsh, Andrew J.; Miranda, Luis F.; +3 Authors

doi: 10.1017/s1743921317010092

handle: 10261/216249

Magnetic fields and radio emission processes in maser-emitting planetary nebulae

Abstract

AbstractWe present polarimetric observations of the 4 ground-state transitions of OH, toward a sample of maser-emitting planetary nebulae (PNe) using the Australia Telescope Compact Array. This sample includes confirmed OH-emitting PNe, confirmed and candidate H2O-maser-emitting PNe. Polarimetric observations provide information related to the magnetic field of these sources. Maser-emitting PNe are very young PNe and magnetic fields are a key ingredient in the early evolution and shaping process of PNe. Our preliminary results suggest that magnetic field strengths may change very rapidly in young PNe.

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Spain
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Keywords

masers, Magnetic fields, Polarization, Stars: AGB and post-AGB, Planetary nebulae: general, AGB and post-AGB [Stars], general [Planetary nebulae]

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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