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Discovery of periodic and alternating flares of the methanol and water masers in G107.298+5.639

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arxiv 1604.00796 v1 pith:W7X5IOA2 submitted 2016-04-04 astro-ph.SR astro-ph.GA

Discovery of periodic and alternating flares of the methanol and water masers in G107.298+5.639

classification astro-ph.SR astro-ph.GA
keywords maserflaresmethanolwaterperiodicstellarcomponentsg107
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Methanol and water vapour masers are signposts of early stages of high-mass star formation but it is generally thought that due to different excitation processes they probe distinct parts of stellar environments. Here we present observations of the intermediate-mass young stellar object G107.298+5.639, revealing for the first time that 34.4 d flares of the 6.7 GHz methanol maser emission alternate with flares of individual features of the 22 GHz water maser. High angular resolution data reveal that a few components of both maser species showing periodic behaviour coincide in position and velocity and all the periodic water maser components appear in the methanol maser region of size of 360 au. The maser flares could be caused by variations in the infrared radiation field induced by cyclic accretion instabilities in a circumstellar or protobinary disc. The observations do not support either the stellar pulsations or the seed photon flux variations as the underlying mechanisms of the periodicity in the source.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Fast Population Leakage in Astronomical Masers: Maser Amplification and Transient Superradiance

    astro-ph.HE 2026-07 reject novelty 5.0

    In a three-level maser model, a fast competing decay channel on the shared upper level does not automatically suppress superradiance; the 6.7 GHz methanol flare in S255IR-NIRS3 can still be reproduced when the leakage...