Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-02T22:36:56.258Z Has data issue: false hasContentIssue false
  • English
  • Français

High Speed CCD Photometry of Flare Stars

Published online by Cambridge University Press:  12 April 2016

Sun-Youp Park  and
Yong-Ik Byun
Sun-Youp Park
Affiliation:
Department of Astronomy, Yonsei University, Seoul, 120-749, Korea
Yong-Ik Byun
Affiliation:
Department of Astronomy, Yonsei University, Seoul, 120-749, Korea

Abstract

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.

Previously, flare stars have been observed by fast two channel photoelectric photometry. We have started an observing program to monitor flare stars using a normal CCD camera via a method called “trailed mode photometry”. For this program, we developed a fully automated trail photometry software.

Type
V. Variability Study
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 203 - 204
Copyright
Copyright © Astronomical Society of the Pacific 2001