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Observed and computed spectral line profiles

Published online by Cambridge University Press:  25 May 2016

Dainis Dravins
Dainis Dravins*
Affiliation:
Lund Observatory, Box 43, S-22100 Lund, Sweden

Abstract

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For the diagnostics of stellar surface structure, studies of “ordinary” line profiles may prove inadequate. However, hydrodynamic models may be constrained by second-order quantities, such as line asymmetries and wavelength shifts (and especially the differential behavior between lines of different excitation potential, ionization stage, and height of formation, as well as by the time dependence).

Information

Type
Session V: “Next Generation Model Atmospheres”
Information
Symposium - International Astronomical Union , Volume 176: Stellar Surface Structure , 1996, pp. 519 - 522
Copyright
Copyright © Kluwer 1996 

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