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- W1560401032 abstract "Spectroscopic echelle observations of V751 Cygni and its nearby surroundings are presented here. Although long-slit observations show the presence of variable emission in the material around the object, the temperature and densities derived from [O II], [O III] and [S II] lines suggest that this material comes from the background and is not connected with the cataclysmic variable. An analysis of the radial velocity of the H line gives an orbital period of 0.144584 days." @default.
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- W1560401032 date "2002-02-01" @default.
- W1560401032 modified "2023-10-03" @default.
- W1560401032 title "THE CATACLYSMIC VARIABLE V751 CYG AT THE EYE OF THE PELICAN NEBULA: EVIDENCE OF A CIRCUMSTELLAR RING?" @default.
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