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Discovery of periodic class II methanol masers associated with G339.986-0.425 region

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arxiv 1512.07998 v1 pith:TNLAFELD submitted 2015-12-25 astro-ph.SR

classification astro-ph.SR
keywords masersacrossg339methanolperiodicassociatedchannelsclass
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abstract

Ten new class II methanol masers from the 6.7-GHz Methanol Multibeam survey catalogues III and IV were selected for a monitoring programme at both 6.7 and 12.2 GHz with the 26m Hartebeesthoek Radio Astronomy Observatory (HartRAO) radio telescope for two years and nine months, from August 2012 to May 2015. In the sample, only masers associated with G339.986-0.425 were found to show periodic variability at both 6.7 and 12.2 GHz. The existence of periodic variation was tested with four independent methods. The analytical method gave the best estimation of the period, which was 246 $\pm$ 1 days. The time series of G339.986-0.425 show strong correlations across velocity channels and between the 6.7 and 12.2 GHz masers. The time delay was also measured across channels and shows structure across the spectrum which is continuous between different maser components.

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Cited by 1 Pith paper

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

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

    astro-ph.HE 2026-07 reject novelty 5.0 of 10

    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...

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