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Paper detail

Chemical spots and their dynamical evolution on HgMn stars

Our recent studies of late B-type stars with HgMn peculiarity revealed for the first time the presence of fast dynamical evolution of chemical spots on their surfaces. These observations suggest a hitherto unknown physical process operating in the stars with radiative outer envelopes. Furthermore, we have also discovered existence of magnetic fields on these stars that have up to now been thought to be non-magnetic. Here we will discuss the dynamical spot evolution on HD 11753 and our new results on magnetic fields on AR Aur.

preprint2010arXivOpen access
Heidi KorhonenSwetlana HubrigMaryline BriquetFederico GonzalezIgor Savanov
astro-ph.SR
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Heidi KorhonenSwetlana HubrigMaryline BriquetFederico GonzalezIgor Savanov

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