Balmer decrement of AG Pegasi
Abstract
The results of the spectrophotometry of emission lines of the star AG Peg are discussed. Twenty spectrograms of this star have been obtained by means of 10" telescope ASI-5 in 1959-1962. It was concluded that considerable variations of Balmer decrement have taken place during the period of observations.
- Publication:
-
Communications of the Byurakan Astrophysical Observatory
- Pub Date:
- 1963
- Bibcode:
- 1963CoBAO..34...93I