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- Title
EMISSION ACTIVITY OF THE Be STAR 60 CYGNI.
- Authors
Šejnová, K.; Votruba, V.
- Abstract
In this paper we present results of spectroscopic analysis of the Hα line profile of the Be star 60 Cygni. We present time evolution of the equivalent width of the Hα line profiles during years 1992 - 2016 and V/R variation during years 1995 - 2016. We analyzed data from Ondřejov Observatory and from BeSS Database. The circumstellar disk of the star was present twice during years 1992 - 2016 and the second cycle shows stronger emission activity. We found out that the formation of the disk takes longer time than the disk extinction (the extinction is much steeper than the formation) and that there is no evident period of changes in the V/R variation.
- Subjects
SPECTROSCOPIC light sources; P Cygni stars; STELLAR evolution; ASTRONOMY; CIRCUMSTELLAR matter
- Publication
Serbian Astronomical Journal, 2017, Issue 194, p51
- ISSN
1450-698X
- Publication type
Article
- DOI
10.2298/SAJ1794051S