Hydrogen emission lines of the symbiotic system AG Peg

Computer Science

Scientific paper

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Emission Spectra, H Lines, Stellar Spectrophotometry, Symbiotic Stars, Balmer Series, Gas Dynamics

Scientific paper

Variations of the intensity and profiles of the hydrogen lines of AG Peg
are examined in order to investigate the gas dynamics in this system.
Data on the variations of these parameters of the hydrogen emission
lines do not provide evidence for the occultation of the gas in which
they excited by the cold component of the system.

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