Modelling the H Lyman lines in evolved late-type stars

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Abstract

The importance of partial redistribution (PRD) in the modelling of the Lyman a and Lyman ß emission lines of hydrogen in stellar atmospheres is examined using simple atmospheric models of a range of late-type stars. These models represent the subgiant Procyon (F5 IV-V), and the two giants ß Gem (K0 III) and a Tau (K5 III). These stars are selected to span a wide range of surface gravities: 1.25 <log g <4.00. The calculations are performed using the computer code MULTI with the modifications made by Hubeny & Lites. It is found that PRD effects are highly significant, both in the direct prediction of the Lyman line profiles and in the application of hydrostatic equilibrium to calculate the atmospheric electron density in static atmospheric models.
Original languageEnglish
Pages (from-to)821-832
Number of pages12
JournalMonthly Notices of the Royal Astronomical Society
Volume326
Issue number2
DOIs
Publication statusPublished - 11 Sep 2001

Bibliographical note

Copyright 2005 Elsevier Science B.V., Amsterdam. All rights reserved.

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