Optical polarimetry study of Lambda-Orionis star-forming region
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arXiv
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| Natura: | Preprint |
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2024
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| _version_ | 1866914950914506752 |
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| author | Neha, Sharma Soam, Archana Maheswar, G. |
| author_facet | Neha, Sharma Soam, Archana Maheswar, G. |
| contents | We present an optical polarimetric study of a nearby star-forming region, Lambda-Orionis, to map plane-of-the-sky magnetic field geometry to understand the magnetized evolution of the HII region and associated small molecular clouds. We made multi-wavelength polarization observations of 34 bright stars distributed across the region. R-band polarization measurements focused on small molecular clouds BRC 17 and BRC 18 located at the periphery of the HII region are also presented. The magnetic field lines exhibit a large-scale ordered orientation consistent with the Planck sub-mm polarization measurements. The magnetic field lines in both the BRCs are found to be roughly in north-south directions; however, a larger dispersion is noticed in the orientation for BRC 17 compared to BRC 18. Using structure-function analysis, the strength of the plane-of-the-sky component of the magnetic field is estimated as $\sim$28 $μ$G for BRC 17 and $\sim$40 $μ$G for BRC 18. The average dust grain size and the mean value of the total-to-selective extinction ratio (R$_{V}$) in the HII region are found to be $\sim$0.51 $\pm$ 0.05 $μ$m and $\sim$2.9 $\pm$ 0.3, respectively. The distance of the whole HII region is estimated as $\sim$392 $\pm$ 8 pc by combining astrometry information from GAIA EDR3 for YSOs associated with BRCs and confirmed members of central cluster Collinder 69. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_02193 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Optical polarimetry study of Lambda-Orionis star-forming region Neha, Sharma Soam, Archana Maheswar, G. Astrophysics of Galaxies Solar and Stellar Astrophysics We present an optical polarimetric study of a nearby star-forming region, Lambda-Orionis, to map plane-of-the-sky magnetic field geometry to understand the magnetized evolution of the HII region and associated small molecular clouds. We made multi-wavelength polarization observations of 34 bright stars distributed across the region. R-band polarization measurements focused on small molecular clouds BRC 17 and BRC 18 located at the periphery of the HII region are also presented. The magnetic field lines exhibit a large-scale ordered orientation consistent with the Planck sub-mm polarization measurements. The magnetic field lines in both the BRCs are found to be roughly in north-south directions; however, a larger dispersion is noticed in the orientation for BRC 17 compared to BRC 18. Using structure-function analysis, the strength of the plane-of-the-sky component of the magnetic field is estimated as $\sim$28 $μ$G for BRC 17 and $\sim$40 $μ$G for BRC 18. The average dust grain size and the mean value of the total-to-selective extinction ratio (R$_{V}$) in the HII region are found to be $\sim$0.51 $\pm$ 0.05 $μ$m and $\sim$2.9 $\pm$ 0.3, respectively. The distance of the whole HII region is estimated as $\sim$392 $\pm$ 8 pc by combining astrometry information from GAIA EDR3 for YSOs associated with BRCs and confirmed members of central cluster Collinder 69. |
| title | Optical polarimetry study of Lambda-Orionis star-forming region |
| topic | Astrophysics of Galaxies Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2406.02193 |