September 27, 2021 Poster Open Access

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

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    <subfield code="a">Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422</subfield>
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    <subfield code="a">&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;

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