A unified Maxwell–Bloch framework for multiperiodic 6.7 GHz methanol flaring in G9.62 + 0.20E

ABSTRACT We analyse a decade of 6.7 GHz methanol monitoring data in G9.62 + 0.20E, confirming the known periodicities of $p_{1} = 241.3 \pm 2.3$ d and $p_{2} = 52.5 \pm 0.3$ d, and identifying three new cycles at $p_{3} = 127.0 \pm 1.6$ d, $p_{4} = 163.9 \pm 2.9$ d, and $p_{5} = 204.1 \pm 1.5$ d. The 241.3-d and 204.1-d periods occur in multiple velocity channels, while the others are confined to single components. Despite their diverse morphologies and time-scales, all flares can be reproduced within a unified Maxwell–Bloch framework operating in the fast-transient superradiance regime, driven by narrow periodic pump excitations. Model fits yield consistent environmental parameters across periodicities (temperatures, collisional time-scales), pointing to broadly uniform physical conditions in the masing region. The discovery of new periodicities and their unified Maxwell–Bloch modelling provide a consistent picture of multiperiodic flaring in G9.62 + 0.20E and support superradiance as a general framework for flaring in maser-hosting regions.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-12-12
DOI
https://doi.org/10.1093/mnras/staf2200
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
0.00

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article

A unified Maxwell–Bloch framework for multiperiodic 6.7 GHz methanol flaring in G9.62 + 0.20E

Yoshihiro Tanabe, Yoshinori Yonekura, Fereshteh Rajabi, Gordon MacLeod et al.
Monthly Notices of the Royal Astronomical Society
Astrophysics and Star Formation Studies
article

A unified Maxwell–Bloch framework for multiperiodic 6.7 GHz methanol flaring in G9.62 + 0.20E

Yoshihiro Tanabe, Yoshinori Yonekura, Fereshteh Rajabi, Gordon MacLeod, T. Rashidi, V. Anari, O. Powles
article en

Abstract

ABSTRACT We analyse a decade of 6.7 GHz methanol monitoring data in G9.62 + 0.20E, confirming the known periodicities of $p_{1} = 241.3 \pm 2.3$ d and $p_{2} = 52.5 \pm 0.3$ d, and identifying three new cycles at $p_{3} = 127.0 \pm 1.6$ d, $p_{4} = 163.9 \pm 2.9$ d, and $p_{5} = 204.1 \pm 1.5$ d. The 241.3-d and 204.1-d periods occur in multiple velocity channels, while the others are confined to single components. Despite their diverse morphologies and time-scales, all flares can be reproduced within a unified Maxwell–Bloch framework operating in the fast-transient superradiance regime, driven by narrow periodic pump excitations. Model fits yield consistent environmental parameters across periodicities (temperatures, collisional time-scales), pointing to broadly uniform physical conditions in the masing region. The discovery of new periodicities and their unified Maxwell–Bloch modelling provide a consistent picture of multiperiodic flaring in G9.62 + 0.20E and support superradiance as a general framework for flaring in maser-hosting regions.

Monthly Notices of the Royal Astronomical SocietyVol. 545(3)
Western University (CA), Yamaguchi University (JP), Hartebeesthoek Radio Astronomy Observatory (ZA), Ibaraki University (JP), Open University of Tanzania (TZ), McMaster University (CA)
Government of Canada, National Astronomical Observatory of Japan, Institut Périmètre de physique théorique, Ministry of Colleges and Universities, Natural Sciences and Engineering Research Council of Canada, Japan Society for the Promotion of Science
Openalex Percentile: Top 72%
Astrophysics and Star Formation Studies
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