No CrossRef data available.
Article contents
The Remarkable Eclipsing Binary TW Draconis
Published online by Cambridge University Press: 09 August 2007
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 analyzed a new photometry of this well-known Algol-like eclipsing binary together with old photoelectric measurements with the aim of better understanding of its orbital period changes and short-time light variations modulating the mean light curve. The analysis has been done by the new method based on the combination of the principal component analysis and robust regression. New spectroscopic observations and radial-velocity curve are also presented.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S240: Binary Stars as Critical Tools & Tests in Contemporary Astrophysics , August 2006 , pp. 567 - 570
- Copyright
- Copyright © International Astronomical Union 2007
References
Draper, P.W.
2001-3, Central Laboratory of the Research Councils, http://www.starlink.ac.uk/splat
Google Scholar
Kim, S.-L., Lee, J.W., Kwon, S.-G., Youn, J.-H., Mkrtichian, D.E., & Kim, C.
2003, A&A
405, 231
Google Scholar
Škoda, P.
1996, Astronomical Data Analysis Software and Systems V, ASP Conf. Series, Vol. 101, G.H. Jacoby & J. Barnes, eds., p. 187Google Scholar
You have
Access