Inhomogeneous distribution of mercury on the surfaces of rapidly rotating HgMn stars

Details Inhomogeneous distribution of mercury on the surfaces of rapidly rotating HgMn stars Inhomogeneous distribution of mercury on the surfaces of rapidly rotating HgMn stars

2005-05-06

arxiv.org/abs/astro-ph/0505124v1

Astronomy and Astrophysics

Astrophysics

6 pages, 3 figures, accepted by Astronomy & Astrophysics

Scientific paper

10.1051/0004-6361:20053123

Starspots are usually associated with the action of magnetic fields at the stellar surfaces. However, recently an inhomogeneous chemical distribution of mercury was found for the mercury-manganese (HgMn) star alpha And -- a well-established member of a non-magnetic subclass of the chemically peculiar stars of the upper main sequence. In this study we present first results of the high-resolution survey of the HgII 3984 resonance line in the spectra of rapidly rotating HgMn stars with atmospheric parameters similar to those of alpha And. We use spectrum synthesis modelling and take advantage of the Doppler resolution of the stellar surfaces to probe horizontal structure of mercury distribution. Clear signatures of spots are found in the HgII 3984 line profiles of HR 1185 and HR 8723. Two observations of the latter star separated by two days give evidence for the line profile variability. We conclude that inhomogeneous distribution of Hg is a common phenomenon for the rapidly rotating HgMn stars in the 13000--13800 K effective temperature range independently of the stellar evolutionary stage. These results establish existence of a new class of spectrum variable spotted B-type stars. It is suggested that the observed Hg inhomogeneities arise from dynamical instabilities in the chemical diffusion processes and are unrelated to magnetic phenomena.

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