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Ultraviolet spectroscopy of the symbiotic star AG Pegasi
High resolution UV spectroscopic observations of the binary symbiotic star AG Peg obtained with the IUE satellite in the periode 1978-81 are analyzed. The variability of the fluxes and the radial velocities of emission lines accordingto orbital phase are presented, The observaions support a binary model with mass transfer from a hot rotationaly unstable subdvarf to a cool M giant.
Creator
- D.
- Komárek, Z.
- Vittone, A.
- François-Antoine Chevrier
Subject
- observations
- ultraviolet spectroscopy
- star AG Pegasi
Type of item
- model:article
Creator
- D.
- Komárek, Z.
- Vittone, A.
- François-Antoine Chevrier
Subject
- observations
- ultraviolet spectroscopy
- star AG Pegasi
Type of item
- model:article
Providing institution
Aggregator
Rights statement for the media in this item (unless otherwise specified)
- http://creativecommons.org/publicdomain/mark/1.0/
Rights
- policy:public
Place-Time
- 201-205
Source
- Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:70
Identifier
- uuid:380f6858-8e68-48ed-9c52-cc513d6d99b0
- https://cdk.lib.cas.cz/client/handle/uuid:380f6858-8e68-48ed-9c52-cc513d6d99b0
- uuid:380f6858-8e68-48ed-9c52-cc513d6d99b0
Format
- bez média
- svazek
Language
- ces
- cze
Providing country
- Czech Republic
Collection name
First time published on Europeana
- 2021-06-01T12:19:28.026Z
Last time updated from providing institution
- 2021-06-01T12:19:28.026Z