Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-12T23:08:48.999Z Has data issue: false hasContentIssue false
  • English
  • Français

The $\delta$ Scuti star 44 Tau: Observations and analysis

Published online by Cambridge University Press:  02 March 2005

Victoria Antoci  and
Michel Breger
Victoria Antoci
Affiliation:
Institut for Astronomy, Vienna University, Türkenschanzstrasse 17, A-1180, Vienna, Austria e-mail: antoci@astro.univie.ac.at
Michel Breger
Affiliation:
Institut for Astronomy, Vienna University, Türkenschanzstrasse 17, A-1180, Vienna, Austria e-mail: antoci@astro.univie.ac.at
Rights & Permissions [Opens in a new window]

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.

Between 2000 and 2003 more than 600 hours of photometric data of the $\delta$ Scuti star 44 Tauri (HD 26322) were collected in Strömgren $v$ and $y$ as well as in Johnson $V$. Observations were carried out at Washington Camp (Arizona), the Sierra Nevada Observatory (Spain) and the Ege University Observatory (Turkey). After analyzing the data with Period98 (Sperl 1998) more than 30 frequencies were found to be significant. We present the data and the results of our observational campaigns.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Methods: data analysistechniques: photometricstars: oscillations (including pulsations)stars: individual: (44 Tau)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS224 , July 2004 , pp. 808 - 811
Copyright
© 2004 International Astronomical Union