HD 24733 is an eclipsing spectroscopic binary

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Abstract

The known spectroscopic binary HD 24 733 is shown to be an eclipsing variable. The accurate value of the orbital period (1.762 838 days) has been determined. According to the photometric data, the system is a β Lyrae type interacting binary.

Original languageEnglish
Pages (from-to)786-788
Number of pages3
JournalAstronomy and Astrophysics
Volume317
Issue number3
Publication statusPublished - Jan 20 1997

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Keywords

  • Binaries: eclipsing
  • Binaries: spectroscopic
  • Stars: individual: HD 24 733

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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