Abstract
Molecular clouds are prime locations to study the process of star formation. These clouds contain filamentary structures and cores, which are crucial sites for the formation of young stars. The star-formation process has been investigated using various techniques, including polarimetry, for tracing magnetic fields. In this small review-cum-short report, we put together the efforts (mainly from the Indian community) to understand the roles of turbulence and magnetic fields in star formation. These are two components of the ISM competing against gravity, which is primarily responsible for the collapse of gas to form stars. We also include attempts made using simulations of molecular clouds to study this competition. Studies on feedback and magnetic fields are combined and listed to understand the importance of the interaction between two energies in setting the current observed star formation efficiency. We have listed available and upcoming facilities with the polarization capabilities needed to trace magnetic fields. We have also stated the importance of ongoing and desired collaborations between Indian communities and facilities abroad to shed more light on the roles of turbulence and magnetic fields in the process of star formation.
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Notes
Also, see related three-dimensional visualizations of the molecular clouds and stellar feedback from two of these groups: https://www.youtube.com/watch?v=lphp13WPflc &t=1s and https://www.youtube.com/watch?v=LeX5e51UkzI.
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Acknowledgements
The research work at the Physical Research Laboratory is funded by the Department of Space, Government of India. AS thanks Dr Archita Rai (KASI, S. Korea) for the help in getting a list of optical/NIR polarimeters. CE acknowledges the financial support from grant RJF/2020/000071 as a part of the Ramanujan Fellowship awarded by the Science and Engineering Research Board (SERB). ASe thanks Sajay Sunny Mathew, Christoph Federrath, and Antoine Marchal for useful discussions.
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Soam, A., Eswaraiah, C., Seta, A. et al. Turbulence and magnetic fields in star formation. J Astrophys Astron 45, 17 (2024). https://doi.org/10.1007/s12036-024-10005-z
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DOI: https://doi.org/10.1007/s12036-024-10005-z