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Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares. / Chen, Xi; Liu, Jun-Ting; Баяндина, Ольга; Song, Shi-Min; Хайбрахманов, Сергей Александрович; Соболев, Андрей Михайлович; Liu, Sheng-Yuan; Chen, Zhi-Wei; Li, Da-Lei; Lin, Bin; Xia, Bo; Shen, Zhi-Qiang; Liu, Tie ; Li, Pak-Shing; Zhang, Xiao-Juan.

в: Communications Physics, Том 8, 249, 12.06.2025.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Chen, X, Liu, J-T, Баяндина, О, Song, S-M, Хайбрахманов, СА, Соболев, АМ, Liu, S-Y, Chen, Z-W, Li, D-L, Lin, B, Xia, B, Shen, Z-Q, Liu, T, Li, P-S & Zhang, X-J 2025, 'Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares', Communications Physics, Том. 8, 249. https://doi.org/10.1038/s42005-025-02140-y

APA

Chen, X., Liu, J-T., Баяндина, О., Song, S-M., Хайбрахманов, С. А., Соболев, А. М., Liu, S-Y., Chen, Z-W., Li, D-L., Lin, B., Xia, B., Shen, Z-Q., Liu, T., Li, P-S., & Zhang, X-J. (2025). Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares. Communications Physics, 8, [249]. https://doi.org/10.1038/s42005-025-02140-y

Vancouver

Chen X, Liu J-T, Баяндина О, Song S-M, Хайбрахманов СА, Соболев АМ и пр. Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares. Communications Physics. 2025 Июнь 12;8. 249. https://doi.org/10.1038/s42005-025-02140-y

Author

Chen, Xi ; Liu, Jun-Ting ; Баяндина, Ольга ; Song, Shi-Min ; Хайбрахманов, Сергей Александрович ; Соболев, Андрей Михайлович ; Liu, Sheng-Yuan ; Chen, Zhi-Wei ; Li, Da-Lei ; Lin, Bin ; Xia, Bo ; Shen, Zhi-Qiang ; Liu, Tie ; Li, Pak-Shing ; Zhang, Xiao-Juan. / Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares. в: Communications Physics. 2025 ; Том 8.

BibTeX

@article{da582a15b7704b58bb06ac0bfc13271d,
title = "Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares",
abstract = "Magnetic reconnection, a critical process in astrophysical luminosity outbursts like solar flares, may also underpin such events in high-mass young stellar objects (HMYSOs). Despite theoretical predictions, observational evidence linking luminosity outbursts to magnetic reconnection in HMYSOs is still lacking. Our study examines the bursting HMYSO G36.11+0.55, where we find a significant correlation between the variability of 6.668 GHz CH3OH maser and the magnetic field strength inferred from 6.035 GHz ex-OH masers. This aligns with models of accretion-driven magnetic flux accumulation and reconnection-driven ejection, proposed for low-mass protostellar flares in theoretical studies. The CH3OH maser light curve closely resembles those observed or expected in other luminosity outbursts linked to magnetic reconnection. Furthermore, CH3OH maser flare regions coincide with jets from the source, also supporting the model of reconnection-driven magnetic flux ejection. These observational results underscore the essential role of magnetic fields in HMYSO outburst dynamics and material accretion near HMYSOs.",
author = "Xi Chen and Jun-Ting Liu and Ольга Баяндина and Shi-Min Song and Хайбрахманов, {Сергей Александрович} and Соболев, {Андрей Михайлович} and Sheng-Yuan Liu and Zhi-Wei Chen and Da-Lei Li and Bin Lin and Bo Xia and Zhi-Qiang Shen and Tie Liu and Pak-Shing Li and Xiao-Juan Zhang",
year = "2025",
month = jun,
day = "12",
doi = "10.1038/s42005-025-02140-y",
language = "English",
volume = "8",
journal = "Communications Physics",
issn = "2399-3650",
publisher = "Springer Nature",

}

RIS

TY - JOUR

T1 - Magnetic reconnection as the driving factor behind high-mass protostellar luminosity flares

AU - Chen, Xi

AU - Liu, Jun-Ting

AU - Баяндина, Ольга

AU - Song, Shi-Min

AU - Хайбрахманов, Сергей Александрович

AU - Соболев, Андрей Михайлович

AU - Liu, Sheng-Yuan

AU - Chen, Zhi-Wei

AU - Li, Da-Lei

AU - Lin, Bin

AU - Xia, Bo

AU - Shen, Zhi-Qiang

AU - Liu, Tie

AU - Li, Pak-Shing

AU - Zhang, Xiao-Juan

PY - 2025/6/12

Y1 - 2025/6/12

N2 - Magnetic reconnection, a critical process in astrophysical luminosity outbursts like solar flares, may also underpin such events in high-mass young stellar objects (HMYSOs). Despite theoretical predictions, observational evidence linking luminosity outbursts to magnetic reconnection in HMYSOs is still lacking. Our study examines the bursting HMYSO G36.11+0.55, where we find a significant correlation between the variability of 6.668 GHz CH3OH maser and the magnetic field strength inferred from 6.035 GHz ex-OH masers. This aligns with models of accretion-driven magnetic flux accumulation and reconnection-driven ejection, proposed for low-mass protostellar flares in theoretical studies. The CH3OH maser light curve closely resembles those observed or expected in other luminosity outbursts linked to magnetic reconnection. Furthermore, CH3OH maser flare regions coincide with jets from the source, also supporting the model of reconnection-driven magnetic flux ejection. These observational results underscore the essential role of magnetic fields in HMYSO outburst dynamics and material accretion near HMYSOs.

AB - Magnetic reconnection, a critical process in astrophysical luminosity outbursts like solar flares, may also underpin such events in high-mass young stellar objects (HMYSOs). Despite theoretical predictions, observational evidence linking luminosity outbursts to magnetic reconnection in HMYSOs is still lacking. Our study examines the bursting HMYSO G36.11+0.55, where we find a significant correlation between the variability of 6.668 GHz CH3OH maser and the magnetic field strength inferred from 6.035 GHz ex-OH masers. This aligns with models of accretion-driven magnetic flux accumulation and reconnection-driven ejection, proposed for low-mass protostellar flares in theoretical studies. The CH3OH maser light curve closely resembles those observed or expected in other luminosity outbursts linked to magnetic reconnection. Furthermore, CH3OH maser flare regions coincide with jets from the source, also supporting the model of reconnection-driven magnetic flux ejection. These observational results underscore the essential role of magnetic fields in HMYSO outburst dynamics and material accretion near HMYSOs.

UR - https://www.mendeley.com/catalogue/49a31d37-d0c4-39a0-85f4-4be3b27dc919/

U2 - 10.1038/s42005-025-02140-y

DO - 10.1038/s42005-025-02140-y

M3 - Article

VL - 8

JO - Communications Physics

JF - Communications Physics

SN - 2399-3650

M1 - 249

ER -

ID: 137080699