Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-14T09:50:23.319Z Has data issue: false hasContentIssue false
  • English
  • Français

On Periodic Variations in the Spectrum of the BOe Star X Persei Associated With the X-Ray Source 3U 0352+30

Published online by Cambridge University Press:  14 August 2015

T.S. Galkina
T.S. Galkina*
Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The bright BOe star X Persei has been observed for over fifthy years, both as an emission line object and as a variable star.

Type
III. Spectroscopy
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 189 - 194
Copyright
Copyright © Reidel 1982