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

A. S. Miroshnichenko; K. S. Bjorkman; V. D. Krugov; I. A. Usenko

doi:10.18524/1810-4215.2001.14.99469

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, United States
K. S. Bjorkman Ritter Observatory, University of Toledo, Toledo, Ohio, 43606, USA, United States
V. D. Krugov Main Astronomical Observatory, Kiev, Ukraine, Ukraine
I. A. Usenko Astronomical Observatory, Odessa National University, Odessa, 65014, Ukraine, Ukraine

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.