Curvature Mapping Method: Mapping Lorentz Force in Orion A
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arXiv
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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| _version_ | 1866911474138480640 |
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| author | Zhao, Mengke Li, Guang-Xing Qiu, Keping |
| author_facet | Zhao, Mengke Li, Guang-Xing Qiu, Keping |
| contents | Magnetic force is a fundamental force in nature. Although widely believed to be important in counterbalancing against collapse in star formation, a clear evaluation of the role of the magnetic field in star formation remains hard to achieve. Past research attempts to evaluate the importance of magnetic forces using diagnostics such as the mass-to-flux ratio, which measures its strength but not how it functions. Since star formation is a complex process and the observed regions have complex structures, mapping the importance of the magnetic field is necessary. We propose a new technique, the Curvature Mapping Method, to evaluate the role of the magnetic force by providing maps of the magnetic force estimated using polarization observations. The Curvature Mapping Method provides maps with the contribution of the magnetic force clearly outlined. We apply the method to the star formation region of Orion A and provide a first quantitative result where the magnetic force arising from the pinched magnetic field does provide support against gravity. By comparing it against the gravitational force, we find that the magnetic force is enough to affect the low-density gas but is insufficient to support the dense region from collapse. The method effectively uses information contained in polarization maps and can be applied to data from surveys to understand the role of the B-field. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2408_09690 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Curvature Mapping Method: Mapping Lorentz Force in Orion A Zhao, Mengke Li, Guang-Xing Qiu, Keping Astrophysics of Galaxies Magnetic force is a fundamental force in nature. Although widely believed to be important in counterbalancing against collapse in star formation, a clear evaluation of the role of the magnetic field in star formation remains hard to achieve. Past research attempts to evaluate the importance of magnetic forces using diagnostics such as the mass-to-flux ratio, which measures its strength but not how it functions. Since star formation is a complex process and the observed regions have complex structures, mapping the importance of the magnetic field is necessary. We propose a new technique, the Curvature Mapping Method, to evaluate the role of the magnetic force by providing maps of the magnetic force estimated using polarization observations. The Curvature Mapping Method provides maps with the contribution of the magnetic force clearly outlined. We apply the method to the star formation region of Orion A and provide a first quantitative result where the magnetic force arising from the pinched magnetic field does provide support against gravity. By comparing it against the gravitational force, we find that the magnetic force is enough to affect the low-density gas but is insufficient to support the dense region from collapse. The method effectively uses information contained in polarization maps and can be applied to data from surveys to understand the role of the B-field. |
| title | Curvature Mapping Method: Mapping Lorentz Force in Orion A |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2408.09690 |