Paschen is partially Back

Author(s)
Martin Stift, Franco Leone
Abstract

We present a discussion of the partial Paschen-Back (PB) effect in magnetic Ap stars. An overview of the theory is illustrated with examples of how splittings deviate non-linearly from the simple Zeeman picture; normally forbidden "ghost lines" appear in strong fields. Resulting asymmetric stellar Stokes profiles for a dipolar magnetic geometry are shown for the Fe II λ 6149 line and it is established that PB lines may be subject to wavelength shifts. Modelling of Stokes profiles in the PB regime opens exciting new diagnostics.

Organisation(s)
Department of Astrophysics
External organisation(s)
Università degli Studi di Catania
Journal
Contributions of the Astronomical Observatory Skalnaté Pleso
Volume
38
Pages
185-190
ISSN
1335-1842
Publication date
2008
Austrian Fields of Science 2012
103004 Astrophysics, 103003 Astronomy
Portal url
https://ucrisportal.univie.ac.at/en/publications/79c928fb-062a-461c-a640-87f535f05cdb