September 27, 2021 Poster Open Access

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

DataCite XML Export

<?xml version='1.0' encoding='utf-8'?>
<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd">
  <identifier identifierType="DOI">10.5281/zenodo.5532717</identifier>
  <creators>
    <creator>
      <creatorName>Volvach, A.E.</creatorName>
      <givenName>A.E.</givenName>
      <familyName>Volvach</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-3839-3466</nameIdentifier>
      <affiliation>Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea</affiliation>
    </creator>
    <creator>
      <creatorName>Volvach, L.N.</creatorName>
      <givenName>L.N.</givenName>
      <familyName>Volvach</familyName>
      <affiliation>Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea</affiliation>
    </creator>
    <creator>
      <creatorName>LArionov, M.G.</creatorName>
      <givenName>M.G.</givenName>
      <familyName>LArionov</familyName>
      <affiliation>Astro Space Center, Lebedev Physical Institute RAS, Moscow</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <subjects>
    <subject>stars: formation –HII regions – ISM: molecules – radio lines: ISM.</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2021-09-27</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5532717</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5532716</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422&lt;br&gt;
&lt;br&gt;
A. E. Volvach &lt;sup&gt;1&lt;/sup&gt;, L. N. Volvach &lt;sup&gt;1&lt;/sup&gt;, M. G. Larionov &lt;sup&gt;2&lt;/sup&gt;&lt;br&gt;
&lt;br&gt;
&lt;sup&gt;1&lt;/sup&gt; Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea&lt;br&gt;
&lt;sup&gt;2&lt;/sup&gt;&amp;nbsp; Astro Space Center, Lebedev Physical Institute RAS, Moscow&lt;/p&gt;

&lt;p&gt;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.&lt;/p&gt;

&lt;p&gt;&amp;nbsp;&lt;/p&gt;</description>
  </descriptions>
</resource>