Volvach, A.E.
Volvach, L.N.
LArionov, M.G.
2021-09-27
<p>Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422<br>
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A. E. Volvach <sup>1</sup>, L. N. Volvach <sup>1</sup>, M. G. Larionov <sup>2</sup><br>
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<sup>1</sup> Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea<br>
<sup>2</sup> Astro Space Center, Lebedev Physical Institute RAS, Moscow</p>
<p>Unique results of detailed (one-two days interval between data) one-year monitoring of the young binary system IRAS 16293-2422, performed on the RT-22 radio telescope (Simeiz), are obtained. For the first time, a short, powerful flare of a water vapor maser was recorded (feature +8 km/s), which is a combination of three components. New data on the parameters of the medium in which maser radiation is formed was obtained.</p>
<p> </p>
https://doi.org/10.5281/zenodo.5532717
oai:zenodo.org:5532717
eng
Zenodo
https://zenodo.org/communities/plato2021
https://doi.org/10.5281/zenodo.5532716
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
stars: formation –HII regions – ISM: molecules – radio lines: ISM.
Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422
info:eu-repo/semantics/conferencePoster