PoS - Proceedings of Science
Volume 368 - The Golden Age of Cataclysmic Variables and Related Objects V (GOLDEN2019) - Classical Novae, Recurrent Novae and Nova-Like Stars
Balmer Decrement and Outburst of Symbiotic Stars
K. Tanabe*, K. Ando and N. Fukuda
Full text: Not available
Balmer decrement defined by the ratio of spectral intensity defined by I(Hα) /I(Hβ) is applied tentatively to the recent outbursts of three symbiotic stars (AG Peg,V 694 Mon and AG Dra). As a result, during the outbursts,a characteristic feature can be recognized between their brightness change (from AAVSO data base) and the Balmer decrement obtained from our low-resolution spectroscopic observational data.The resulting feature seems to coincide partially with the formula derived from the simplified theory based on the Rayleigh scattering.
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.