The high amplitude delta Scuti star SZ Lyncis revisited

M. Paparó, B. Szeidl, Hamid A. Mahdy

Research output: Contribution to journalArticle

19 Citations (Scopus)

Abstract

Nine new times of light maximum are given for SZ Lyn and the time base of observations is herewith extended to 26 years. 154 light maxima have been used to calculate the orbital elements and the secular change in the period of the pulsating component. The results provided here support the post-Main Sequence, high mass hypothesis for the evolutionary state of this dwarf cepheid.

Original languageEnglish
Pages (from-to)73-82
Number of pages10
JournalAstrophysics and Space Science
Volume149
Issue number1
DOIs
Publication statusPublished - Nov 1 1988

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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