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Fine structure and refractive scattering of the H2O maser in star-forming region W49N
Published online by Cambridge University Press: 07 February 2024
Abstract
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We used the unprecedented resolution of ∼25 μas of the VLBI array formed with the RadioAstron satellite to study the structures of H2O maser spots in the star forming region W49N. We found that anisotropic diffractive scattering of the ISM dominates the images of the maser spot, but does not completely blur them. The refractive scattering floor is about 0.001 in visibility at a baseline of 8 Gλ.
- Type
- Poster Paper
- Information
- Proceedings of the International Astronomical Union , Volume 18 , Symposium S380: Cosmic Masers: Proper Motion toward the Next-Generation Large Projects , December 2022 , pp. 238 - 239
- Copyright
- © The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union
References
Zhang, B., Reid, M. J., Menten, K. M., et al. 2013, ApJ, 775, 1
10.1088/0004-637X/775/1/79CrossRefGoogle Scholar
Deshpande, A. A., Goss, W. M., Mendoza-Torres, J. E. 2013, ApJ, 775, 36
10.1088/0004-637X/775/1/36CrossRefGoogle Scholar
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