Context. The G25. 65+ 1.04 source is one of the few known 'super-flare'water masers in the Milky Way, but in contrast to other super-flare sources, it remains the least studied. In fact …
JH Wu, X Chen, YK Zhang, SP Ellingsen… - The Astrophysical …, 2023 - iopscience.iop.org
We have conducted a systematic line survey, primarily focused on transitions of the methanol and ammonia molecules, and monitoring observations of masers toward the high …
OS Bayandina, RA Burns, SE Kurtz… - The Astrophysical …, 2019 - iopscience.iop.org
Abstract The source G25. 65+ 1.05 (RAFGL7009S, IRAS 18316-0602) is the least studied of the three regions of massive star formation known to show exceptionally powerful H 2 O …
P Jaroenjittichai, K Sugiyama, BH Kramer… - arXiv preprint arXiv …, 2022 - arxiv.org
This White Paper summarises potential key science topics to be achieved with Thai National Radio Telescope (TNRT). The commissioning phase has started in mid 2022. The key …
AE Volvach, LN Volvach, MG Larionov - Journal of Astrophysics and …, 2024 - Springer
Several powerful flare events have been recorded because of long-term monitoring on the RT-22 radio telescope (Simeiz) of the galactic source G25. 65\(+\) 1.05 from 2000 to 2024 …
AM Sobolev, AP Bisyarina, SY Gorda… - … in Astronomy and …, 2019 - iopscience.iop.org
We report variation of K-band infrared (IR) emission in the vicinity of the G025. 65+ 1.05 water and methanol maser source. New observational data were obtained with the 2.5 m …
Outburst or flare in maser activities around star-forming regions provide intriguing clues into the ongoing star formation activities in the region. Flares have been observed in a number of …