HD 210111 compared to FG Vir and θ2 Tau: a test to the λ Bootis phenomenon

Autor(en)

Paul Beck

Abstrakt

The ? Bootis stars are a spectroscopic subgroup of chemically peculiar Population I A-type stars. They show significant underabundances of Fe-peak elements and solar abundances of lighter elements. Theoretical explanations include surface phenomena and binarity. We compared the pulsating ? Bootis star HD 210111 with two normal ? Scuti pulsators. This comparison shows that the pulsational behaviour of HD 210111 is compatible with the ? Bootis phenomenon being a surface effect only.

Organisation(en)

Institut für Astrophysik

Journal

Journal of Physics: Conference Series

Band

118

ISSN

1742-6588

DOI

https://doi.org/10.1088/1742-6596/118/1/012046

Publikationsdatum

2008

ÖFOS 2012

1030 Physik, Astronomie

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/0de08d39-9bc0-481e-a459-cf941043050b