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New Methanol Maser Transitions and Maser Variability Identified from an Accretion Burst Source G358.93-0.03

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Заглавие New Methanol Maser Transitions and Maser Variability Identified from an Accretion Burst Source G358.93-0.03
 
Автор Miao, D.
Chen, X.
Song, S. -M.
Sobolev, A. M.
Breen, S. L.
MacLeod, G. C.
Li, B.
Parfenov, S.
Bisyarina, A.
Shen, Z. -Q.
 
Описание The high-mass young stellar object G358.93-0.03 underwent an accretion burst during the period from 2019 January to June. Given its extraordinary conditions, a number of new maser transitions may have been naturally excited during the burst stage. Searching for new maser lines and monitoring maser variability associated with the accretion burst event are important for understanding the complex conditions of the massive star formation toward G358.93-0.03. In this work, using the Shanghai 65 m Tianma Radio Telescope, we continuously monitored the multiple maser (including methanol and water) transitions toward G358.93-0.03 during the burst in the period from 2019 March 14 to May 20. There were 23 CH3OH maser transitions and one H2O maser transition detected from the monitoring. Nearly all the detected maser transitions toward this source have dramatic variations in their intensities within a short period of ∼2 months. Eight new methanol transitions from G358.93-0.03 were identified to be masering in our observations based on their spectral profile, line width, intensity, and the rotation diagram. During the monitoring, the gas temperature of the clouds in the case of saturated masers can show a significant decline, indicating that the maser clouds were going through a cooling process, possibly associated with the propagation of a heat wave induced by the accretion burst. Some of the maser transitions were even detected with the second flares in 2019 April, which may be associated with the process of the heat-wave propagation induced by the same accretion burst acting on different maser positions. © 2022. The Author(s). Published by the American Astronomical Society.
Russian Ministry of Science and Higher Education Theoretical, (075-15-2020-780, 780–10)
National Natural Science Foundation of China, NSFC, (11590781, 11873002, 12011530065)
This work is supported by the National Natural Science Foundation of China (11873002, 12011530065, 11590781). X.C. thanks Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme (2019). A.M.S. was supported by the Large Scientific Project of the Russian Ministry of Science and Higher Education Theoretical and experimental studies of the formation and evolution of extrasolar planetary systems and characteristics of exoplanets (No. 075-15-2020-780, contract 780–10).
 
Дата 2024-04-22T15:52:54Z
2024-04-22T15:52:54Z
2022
 
Тип Article
Journal article (info:eu-repo/semantics/article)
Published version (info:eu-repo/semantics/publishedVersion)
 
Идентификатор Miao, D, Chen, X, Song, S, Sobolev, AM, Breen, SL, Macleod, GC, Li, B, Parfenov, S, Bisyarina, A & Shen, Z 2022, 'New Methanol Maser Transitions and Maser Variability Identified from an Accretion Burst Source G358.93-0.03', Astrophysical Journal, Supplement Series, Том. 263, № 1, 9, стр. 9. https://doi.org/10.3847/1538-4365/ac9524
Miao, D., Chen, X., Song, S., Sobolev, A. M., Breen, S. L., Macleod, G. C., Li, B., Parfenov, S., Bisyarina, A., & Shen, Z. (2022). New Methanol Maser Transitions and Maser Variability Identified from an Accretion Burst Source G358.93-0.03. Astrophysical Journal, Supplement Series, 263(1), 9. [9]. https://doi.org/10.3847/1538-4365/ac9524
0067-0049
Final
All Open Access; Gold Open Access
https://iopscience.iop.org/article/10.3847/1538-4365/ac9524/pdf
https://iopscience.iop.org/article/10.3847/1538-4365/ac9524/pdf
http://elar.urfu.ru/handle/10995/132366
10.3847/1538-4365/ac9524
85142483276
882598200001
 
Язык en
 
Права Open access (info:eu-repo/semantics/openAccess)
cc-by
 
Формат application/pdf
 
Издатель American Astronomical Society
 
Источник The Astrophysical Journal Supplement Series
Astrophysical Journal, Supplement Series