A new way to calculate doublet P-Cygni profiles

Research output: Chapter in Book/Report/Conference proceedingConference paper

Abstract

A new way to calculate doublet P-Cygni profiles in comoving frame was used to calculate theoretical C IV profiles for early type stars in the Magellanic Clouds. The calculated profiles were compared to the profile fits presented by Patriarchi et al. (1992). Two examples are shown: HD 268605 and HD 169698.
Original languageEnglish
Title of host publicationNew Aspects of Magellanic Cloud research
EditorsBodo Baschek, Gerhard Klare, James Lequeux
PublisherSpringer
Pages278-279
Number of pages2
Volume416
Publication statusPublished - 1993
EventUnknown -
Duration: 1 Jan 1993 → …

Publication series

NameLecture Notes in Physics

Conference

ConferenceUnknown
Period1/01/93 → …

Bibliographical note

Bodo Baschek, Gerhard Klare, James Lequeux

Keywords

  • EARLY STARS
  • STELLAR WINDS

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