Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap.....39..208m&link_type=abstract
Astrophysics, Volume 39, Issue 3, pp.208-215
Astronomy and Astrophysics
Astrophysics
4
Scientific paper
Measurements of radial velocities from the SiII λ6347A and λ6371Alines and the HeI λ6678A line based on observations of 1989 1994 are examined. The variability of the line shapes over the 96.6-day orbital period is analyzed. Evidence for a second component is found from lines in the spectrum of α And which correspond to the silicon lines λ6347 and λ6371A. The preliminary value for the rotational velocity of the secondary component is 100 120 km/sec. Analysis of the variability of the radial velocities of the HeI λ6678A line during the night has given the rotational period of the star of Prot=Id.012344 and indicates an inhomogeneous distribution either of the helium abundance or of the physical conditions over the surface. Thus, we have the first evidence for the existence of spots on the surface of an HgMn star.
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