In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 54, no. 2
M. Tomova - K. Stoyanov - Y. Nikolov - P. Kaygorodov
Detaily:
Rok, strany: 2024, 186 - 189
Jazyk: eng
Kľúčové slová:
binaries: symbiotic, stars: mass-loss, stars: individual: RS Oph
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2024/Vol_54/No_2/pp186-189_abstract.html
O článku:
RS Oph is a recurrent symbiotic novae which underwent its last optical eruption in August 2021. The early Hα spectroscopy of the system (at days 11--15 of the outburst) reveals satellite line components at the velocity position of about ±2400 km s-1 which are an indication of bipolar collimated outflow. We derived some parameters of the outflows and system's components and their evolution during our observation.
Ako citovať:
ISO 690:
Tomova, M., Stoyanov, K., Nikolov, Y., Kaygorodov, P. 2024. Optical observations of RS Oph after its 2021 outburst. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 54, no.2, pp. 186-189. 1335-1842. DOI: https://doi.org/10.31577/caosp.2024.54.2.186
APA:
Tomova, M., Stoyanov, K., Nikolov, Y., Kaygorodov, P. (2024). Optical observations of RS Oph after its 2021 outburst. Contributions of the Astronomical Observatory Skalnaté Pleso, 54(2), 186-189. 1335-1842. DOI: https://doi.org/10.31577/caosp.2024.54.2.186
O vydaní:
Vydavateľ: Astronomical Institute, Slovak Academy of Sciences
Publikované: 1. 2. 2024
Verejná licencia:
