Analysis of the magnetic fields in massive young stellar objects with masers
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arXiv
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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2025
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| _version_ | 1866915615405506560 |
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| author | Pavlova, P. I. Khaibrakhmanov, S. A. Sobolev, A. M. |
| author_facet | Pavlova, P. I. Khaibrakhmanov, S. A. Sobolev, A. M. |
| contents | We analyze observational data on methanol masers in the disks of young massive stellar objects in the massive star formation regions: NGC6334I, G33.641-0.228, G12.89+0.49. Special attention is paid to analysis of the magnetic fields and their possible connection with maser flares. For this purpose, we estimate the distance from star to maser, the magnetospheric radius and magnetic field strength in the region of this radius. The distances from stars to masing regions lie in range from 380 to 620 au. Stellar and disk's magnetic field strengths are comparable at the magnetosphere boundary and lie in the range from 590 to 1880 G for considered objects. Our estimates show that the magnetic fields may play an important role in the considered regions. In particular, observed luminosity bursts and maser flares may be related to magnetic reconnection events near the stars. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2511_10186 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Analysis of the magnetic fields in massive young stellar objects with masers Pavlova, P. I. Khaibrakhmanov, S. A. Sobolev, A. M. Solar and Stellar Astrophysics Astrophysics of Galaxies We analyze observational data on methanol masers in the disks of young massive stellar objects in the massive star formation regions: NGC6334I, G33.641-0.228, G12.89+0.49. Special attention is paid to analysis of the magnetic fields and their possible connection with maser flares. For this purpose, we estimate the distance from star to maser, the magnetospheric radius and magnetic field strength in the region of this radius. The distances from stars to masing regions lie in range from 380 to 620 au. Stellar and disk's magnetic field strengths are comparable at the magnetosphere boundary and lie in the range from 590 to 1880 G for considered objects. Our estimates show that the magnetic fields may play an important role in the considered regions. In particular, observed luminosity bursts and maser flares may be related to magnetic reconnection events near the stars. |
| title | Analysis of the magnetic fields in massive young stellar objects with masers |
| topic | Solar and Stellar Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2511.10186 |