Poster Open Access

Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422

Volvach, A.E.; Volvach, L.N.; LArionov, M.G.


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  <dc:creator>Volvach, A.E.</dc:creator>
  <dc:creator>Volvach, L.N.</dc:creator>
  <dc:creator>LArionov, M.G.</dc:creator>
  <dc:date>2021-09-27</dc:date>
  <dc:description>Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422

A. E. Volvach 1, L. N. Volvach 1, M. G. Larionov 2

1 Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea
2  Astro Space Center, Lebedev Physical Institute RAS, Moscow

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.

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  <dc:identifier>https://zenodo.org/record/5532717</dc:identifier>
  <dc:identifier>10.5281/zenodo.5532717</dc:identifier>
  <dc:identifier>oai:zenodo.org:5532717</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>doi:10.5281/zenodo.5532716</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:subject>stars: formation –HII regions – ISM: molecules – radio lines: ISM.</dc:subject>
  <dc:title>Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
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