Light variations of the B star HR 7556 - (Letter to the Editor)

Research output: Contribution to journalLetter


On the basis of new U BV photometry this paper reports on the discovery of the variability of the B star HR 7556. The ellipsoidal character of the light curve indicates that it is probably a long period (P ∼ 40 d ) interacting binary. This interpretation has been confirmed by available radial velocity data.

Original languageEnglish
Pages (from-to)195-199
Number of pages5
JournalAstrophysics and Space Science
Issue number1
Publication statusPublished - Oct 1995

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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