Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-30T14:50:00.254Z Has data issue: false hasContentIssue false
  • English
  • Français

On the induced activity of red dwarfs in close binary systems

Published online by Cambridge University Press:  14 March 2005

N.R. Ikhsanov
N.R. Ikhsanov
Affiliation:
Korea Astronomy Observatory, Taejon, Korea, email: ikhsanov@kao.re.kr Central Astronomical Observatory, Pulkovo 65-1, 196140 St. Petersburg, Russia
Rights & Permissions [Opens in a new window]

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.

AE Aquarii is a star with unique flaring activity. It is a close binary system, which contains a K3V-K5V red dwarf (secondary) and a magnetized white dwarf rotating with the period of 33 s (primary). It is traditionally classified as a peculiar nova-like star and assigned to the DQ Her subclass of magnetic Cataclysmic Variables (CVs).To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 683 - 684
Copyright
© 2004 International Astronomical Union