Maser flares driven by isothermal shock waves

MD Gray, S Etoka, B Pimpanuwat… - Monthly Notices of the …, 2024 - academic.oup.com
We use 3D computer modelling to investigate the time-scales and radiative output from
maser flares generated by the impact of shock waves on astronomical unit-scale clouds in …

Large-scale Effect of an Accretion Burst in the High-Mass Young Stellar Object G358. 93-0.03-MM1

D Miao, X Chen, OS Bayandina… - The Astronomical …, 2024 - iopscience.iop.org
The high-mass young stellar object G358. 93-0.03-MM1 underwent a rapid accretion burst
event from 2019 January to June, resulting in flares observed in most class II methanol …

Maser flares driven by variations in pumping and background radiation

MD Gray, S Etoka, A Travis… - Monthly Notices of the …, 2020 - academic.oup.com
We simulate maser flares by varying either the pump rate or the background level of
radiation in a 3D model of a maser cloud. We investigate the effect of different cloud shapes …

РТ-22 КрАО-патрулирование мазерных H2O источников

ЛН Вольвач, АЕ Вольвач, МГ Ларионов… - …, 2019 - elibrary.ru
Представлены результаты систематических наблюдений выборки ярких мазеров H2O
(G25. 65++ 1.05, G25. 825-0.178, G27. 184-0.082, G34. 403+ 0.233, G35. 20-0.74, G43. 8 …

RadioAstron reveals super-compact structures in the bursting H2O maser source G25. 65+ 1.05

OS Bayandina, NN Shakhvorostova, AV Alakoz… - Advances in Space …, 2020 - Elsevier
Water masers are well-known to be variable on a variety of time scales, but only three
Galactic H 2 O masers are known to flare to the level of 10 5–10 6 Jy (TB∼ 10 17 K): Orion …

Observations of H2O and OH masers in star-forming regions

G Rudnitskij, N Ashimbaeva, O Bayandina… - Proceedings of the …, 2018 - cambridge.org
We report long-term observations of H2O and OH maser emission sources at wavelengths of
1.35 and 18 cm associated with star-forming regions. Strong quasi-periodic flares of maser …