Paschen is Partially Back
Astrophysics
2010-11-26 v1
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 FeII 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.
Cite
@article{arxiv.0801.2738,
title = {Paschen is Partially Back},
author = {M. J. Stift and F. Leone},
journal= {arXiv preprint arXiv:0801.2738},
year = {2010}
}
Comments
6 pages, 3 figures