On the further observations of BE/shell star V 923 AQL

Details On the further observations of BE/shell star V 923 AQL On the further observations of BE/shell star V 923 AQL

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222..191d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 191-203

Astronomy and Astrophysics

Astrophysics

2

B Stars, Binary Stars, H Alpha Line, Infrared Spectra, Visible Spectrum, Balmer Series, H Beta Line, Iue, Radial Velocity

Scientific paper

V 923 Aql is one of the candidate Be stars to be binary star.
In this research, optical and near-infrared spectral measurements of V
923 Aql is presented. V 923 Aql presents variable H Balmer line profiles
with shell components. H alpha profiles present R/V, E/C and radial
velocity variation. Shell parameters of the envelope are calculated.

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