Probing the magnetic fields of massive star forming regions with methanol maser polarisation

Abstract

Methanol masers can provide valuable insight into the processes involved in high-mass star formation, however the local environment in which they form is still unclear. Four primary, yet conflicting, models have emerged to explain the commonly observed methanol maser structures at 6.67 GHz. These suggest that masers trace accretion disks, outflows, shock fronts or disks dominated by infall/outflows. One proposed means of testing these models is through mapping the local magnetic field structures around maser sources, which were predicted to lie parallel to shock and outflows and perpendicular to accretion disks. To follow up this suggestion we have determined magnetic field directions from full polarisation observations of 10 6.67-GHz sources. We find morphology that is parallel to the source structure, indicative of shocks or outflows, in five sources and perpendicular morphology indicative of disks in three. These results do not support any of the expected models and the diverse morphologies observed indicate that the masers could be emitting from different evolutionary stages or environments, or from a common local environment with complex associated magnetic fields. To resolve this conflict we suggest a new approach that will search the simulations of massive star formation, which are just becoming available, for suitable sites for maser emission.

Accepted in MNRAS

References in corpus (8)

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Cited by in corpus (7)

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• The Extraordinary Outburst in the Massive Protostellar System NGC6334I-MM1: Emergence of Strong 6.7 GHz Methanol Masers
• Review of Zeeman Effect Observations of Regions of Star Formation
• EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions III. The flux-limited sample
• EVN observations of 6.7-GHz methanol maser polarization in massive star-forming regions II. First statistical results
• Methanol masers reveal the magnetic field of the high-mass protostar IRAS 18089-1732
• EVN observations of 6.7 GHz methanol maser polarization in massive star-forming regions. V. Completion of the flux-limited sample