The deforming effects of stellar magnetic fields on spectral line profiles

Details The deforming effects of stellar magnetic fields on spectral line profiles The deforming effects of stellar magnetic fields on spectral line profiles

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224..609g&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Physics

Line: Formation, Line: Profiles, Stars: Magnetic Fields, Techniques: Polarimetric.

Scientific paper

The profile of a stellar spectral line is formed by the transfer of
radiation through the atmosphere by atomic processes in different
chemical elements distributed usually unequally over the surface of a
magnetic star.

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