Published September 27, 2021
| Version v1
Poster
Open
Detailed monitoring of the water vapor maser in the binary protostellar system of solar masses IRAS 16293-2422
Creators
- 1. Radio Astronomy of Crimean Astrophysical Observatory RAS, Katsively, Crimea
- 2. Astro Space Center, Lebedev Physical Institute RAS, Moscow
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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volvach_ PLATO2021_full.pdf
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