Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-29T21:40:47.724Z Has data issue: false hasContentIssue false
  • English
  • Français

Re-classification of ROTSE-I δ Scuti stars

Published online by Cambridge University Press:  12 April 2016

H. Jin ,
S.-L. Kim ,
C.-U. Lee ,
D.-J. Lee  and
K.-S. Kim
H. Jin
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
S.-L. Kim
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
C.-U. Lee
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
D.-J. Lee
Affiliation:
Korea Astronomy Observatory, Daejeon, 305-348, Korea
K.-S. Kim
Affiliation:
Department of Astronomy and Space Science, Kyunghee University, Yongin, 449-701, 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.

We present new multiband photometric results for ROTSE-I δ Sct stars and the Fourier decomposition analysis. Our result shows that most of the stars classified as ROTSE-I δ Sct stars seem to be W UMa type eclipsing variable stars.

Type
Part 4. Early-type stars: B, A and F pulsators
Information
International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 279 - 282
Copyright
Copyright © Astronomical Society of the Pacific 2004

References

Jin, H. et al. 2003, A&A, 404, 621 Google Scholar
Morgan, S.M. 2003, PASP, 115, 1250 Google Scholar
Poretti, E. 2001, A&A, 371, 986 Google Scholar