In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no. 2
A. Baklanov - D. Baklanova
Detaily:
Rok, strany: 2019, 341 - 345
Jazyk: eng
Kľúčové slová:
cataclysmic variables, accretion, stars: individual: V1432 Aql
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2019/Vol_49/No_2/pp341-345_abstract.html
O článku:
We present the results of our research of the eclipsing asynchronous polar V1432 Aql. Photometric observations were obtained during 21 nights in 2017-2018 using the 38-cm telescope of the Crimean Astrophysical Observatory. We obtained 22 moments of dips associated with the orbital variability of the binary system and 40 minima associated with self-eclipses of accretion columns in the binary system. We found out that accretion in the system occurs at least on three accreting areas. According to our observations, the spin period of the white dwarf is 0.1405429(102) days in 2017 and 0.1404547(29) days in 2018. The improved orbital period is 0.140234676(15) days.
Ako citovať:
ISO 690:
Baklanov, A., Baklanova, D. 2019. Photometric study of the asynchronous polar V1432 Aql in 2017-2018 at the Crimean Astrophysical Observatory. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 49, no.2, pp. 341-345. 1335-1842.
APA:
Baklanov, A., Baklanova, D. (2019). Photometric study of the asynchronous polar V1432 Aql in 2017-2018 at the Crimean Astrophysical Observatory. Contributions of the Astronomical Observatory Skalnaté Pleso, 49(2), 341-345. 1335-1842.
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 5. 2019
Verejná licencia:
