Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.240..637g&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 240, Oct. 1, 1989, p. 637-645.
Astronomy and Astrophysics
Astronomy
3
B Stars, H Alpha Line, Variable Stars, Emission Spectra, Error Analysis, Radial Velocity, Standard Deviation
Scientific paper
In order to search for rapid V/R variability in the Be star, Eta Cen, a series of H-alpha profiles of this star were observed on three nights between May 28 and June 3, 1986. A method of estimating the standard deviation value (sigma) of V/R ratio measurements is described. From the results of the H-alpha profiles, it was found that few profiles displayed rapid V/R variations which were beyond the 3-sigma limit, with no rapid variations of equivalent widths and peak separations of the two emission components. It was also found that rapid V/R and radial velocity variations of the H-alpha profiles were in close agreement. Low-amplitude night-to-night variations of the V/R ratio were also present in Eta Cen during the interval of the observations.
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