PROPERTIES OF CLASSICAL Be STARS FROM ANALYSIS OF HIGH-RESOLUTION H PROFILES

Автор(и)

  • A. S. Miroshnichenko Ritter Observatory, University of Toledo, Toledo, Ohio, 43606, USA; Pulkovo Observatory, Saint-Petersburg, 196140, Russia, США
  • K. S. Bjorkman Ritter Observatory, University of Toledo, Toledo, Ohio, 43606, USA, США
  • V. D. Krugov Main Astronomical Observatory, Kiev, Ukraine, Україна
  • I. A. Usenko Astronomical Observatory, Odessa National University, Odessa, 65014, Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2001.14.99469

Ключові слова:

stars, Be-stars - stars, binary.

Анотація

We summarize results of the 25 year period of observations of Be-stars. We suggest that Be stars with moderate and strong Hα emission are good candidates to search for binary systems.

Посилання

Reig P., Fabregat J., CoeM.J.: 1997, AsAp., 322,193

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Опубліковано

2017-04-20

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