Second Outburst of the Yellow Symbiotic Star LT Delphini
- Авторы: Ikonnikova N.P.1, Komissarova G.V.1, Arkhipova V.P.1
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Учреждения:
- Sternberg Astronomical Institute
- Выпуск: Том 45, № 6 (2019)
- Страницы: 361-370
- Раздел: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191316
- DOI: https://doi.org/10.1134/S1063773719050025
- ID: 191316
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Аннотация
We present the results of our photoelectric UBV observations of the yellow symbiotic star LT Del over 2010–2018. The binary system LT Del, which consists of a bright K giant and a compact hot star with a temperature of ~100 000 K, has an orbital period of 476 days. In 2017 the variable experienced a second low-amplitude (ΔV ~ 0ṃ7) outburst in the history of its studies whose maximum occurred at an orbital phase of 0.15±0.05. The outburst duration was ~60 days. The B–V and U–B colors in the outburst became noticeably bluer. A difference in the photometric behavior of the star in the 1994 and 2017 outburst has been detected. In the orbital cycle preceding the 2017 outburst a secondary minimum with a depth of 0ṃ7 and 0ṃ20 appeared in the B and V light curves, respectively, whose cause is discussed. The phase light and color curves are presented and explained; the position of the star on the color-color diagram is interpreted. We have estimated the parameters of the cool and hot components of the system based on the distance determination from Gaia DR2.
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Об авторах
N. Ikonnikova
Sternberg Astronomical Institute
Автор, ответственный за переписку.
Email: ikonnikova@gmail.com
Россия, Universitetskii pr. 13, Moscow, 119992
G. Komissarova
Sternberg Astronomical Institute
Email: ikonnikova@gmail.com
Россия, Universitetskii pr. 13, Moscow, 119992
V. Arkhipova
Sternberg Astronomical Institute
Email: ikonnikova@gmail.com
Россия, Universitetskii pr. 13, Moscow, 119992
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