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Analysis of Methanol Maser Flares in G107.298+5.63 andS255-NIRS3

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arxiv 2006.13124 v1 pith:PARWR6ZV submitted 2020-06-23 astro-ph.SR astro-ph.GA

Analysis of Methanol Maser Flares in G107.298+5.63 andS255-NIRS3

classification astro-ph.SR astro-ph.GA
keywords maserflareslightmodelsaturationthreeanalysisands255-nirs3
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A 3D maser model has been used to perform an inverse problem on the light curves from three high-amplitude maser flares, selected on the basis of contemporaneous infra-red observations. Plots derived from the model recover the size of the maser cloud, and two parameters linked to saturation, from three observational properties of the light curve. Recovered sizes are consistent with independent interferometric measurements. Maser objects transition between weak and moderate saturation during a flare.

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