Standard

Fine structure and refractive scattering of the H2O maser in star-forming region W49N. / Shakhvorostova, N. N.; Moran, J. M.; Alakoz, A. V. и др.
в: Proceedings of the International Astronomical Union, Том 18, № S380, 01.12.2022, стр. 238-239.

Результаты исследований: Вклад в журнал › Материалы конференции › Рецензирование

Harvard

Shakhvorostova, NN, Moran, JM, Alakoz, AV, Imai, H, Gwinn, CR & Sobolev, AM 2022, 'Fine structure and refractive scattering of the H2O maser in star-forming region W49N', Proceedings of the International Astronomical Union, Том. 18, № S380, стр. 238-239. https://doi.org/10.1017/S1743921323003460

APA

Shakhvorostova, N. N., Moran, J. M., Alakoz, A. V., Imai, H., Gwinn, C. R., & Sobolev, A. M. (2022). Fine structure and refractive scattering of the H2O maser in star-forming region W49N. Proceedings of the International Astronomical Union, 18(S380), 238-239. https://doi.org/10.1017/S1743921323003460

Vancouver

Shakhvorostova NN, Moran JM, Alakoz AV, Imai H, Gwinn CR, Sobolev AM. Fine structure and refractive scattering of the H2O maser in star-forming region W49N. Proceedings of the International Astronomical Union. 2022 дек. 1;18(S380):238-239. doi: 10.1017/S1743921323003460

Author

Shakhvorostova, N. N. ; Moran, J. M. ; Alakoz, A. V. и др. / Fine structure and refractive scattering of the H2O maser in star-forming region W49N. в: Proceedings of the International Astronomical Union. 2022 ; Том 18, № S380. стр. 238-239.

BibTeX

@article{868f3b562b3a4f82995b27f0b3e42eab,
title = "Fine structure and refractive scattering of the H2O maser in star-forming region W49N",
abstract = "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.",
author = "Shakhvorostova, {N. N.} and Moran, {J. M.} and Alakoz, {A. V.} and H. Imai and Gwinn, {C. R.} and Sobolev, {A. M.}",
year = "2022",
month = dec,
day = "1",
doi = "10.1017/S1743921323003460",
language = "English",
volume = "18",
pages = "238--239",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S380",

}

RIS

TY - JOUR

T1 - Fine structure and refractive scattering of the H2O maser in star-forming region W49N

AU - Shakhvorostova, N. N.

AU - Moran, J. M.

AU - Alakoz, A. V.

AU - Imai, H.

AU - Gwinn, C. R.

AU - Sobolev, A. M.

PY - 2022/12/1

Y1 - 2022/12/1

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85185764886

U2 - 10.1017/S1743921323003460

DO - 10.1017/S1743921323003460

M3 - Conference article

VL - 18

SP - 238

EP - 239

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S380

ER -

ID: 53846398