Two periods instead of one in a single 6.7 GHz methanol maser feature in G9.62+0.20E
Abstract
The source G9.62+0.20E surprises yet again! Analysis of the associated methanol maser feature at vlsr = +8.8 km s-1 revealed a second period of P = 52.1 ± 0.3 d, along with the previously reported period P = 243 d for this source. Various explanations, harmonic flaring, Dicke's superradiance, a secondary pulsation, or two different periodically varying radio sources in the field of view with associated methanol masers are presented. The latter two hypotheses appear more plausible but it is not clear which, if any, best describe these observations.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- October 2022
- DOI:
- 10.1093/mnrasl/slac083
- Bibcode:
- 2022MNRAS.516L..96M
- Keywords:
-
- masers;
- stars: formation;
- stars: protostars;
- ISM: individual objects: G9.62+0.20E;
- ISM: molecules;
- radio lines: ISM