Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-12T08:36:51.468Z Has data issue: false hasContentIssue false
  • English
  • Français

Scanner observations of some close binary systems

Published online by Cambridge University Press:  04 August 2017

D. J. Sullivan ,
M. Walkington  and
E. Budding
D. J. Sullivan
Affiliation:
Physics Department, Victoria University of Wellington, and Carter Observatory Wellington, NEW ZEALAND
M. Walkington
Affiliation:
Physics Department, Victoria University of Wellington, and Carter Observatory Wellington, NEW ZEALAND
E. Budding
Affiliation:
Physics Department, Victoria University of Wellington, and Carter Observatory Wellington, NEW ZEALAND

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.

Using our intermediate bandwidth photometric scanner, we have obtained light curve data at a range of spectral intervals for a number of close eclipsing binary systems. This paper reports briefly on the instrumentation system, the data obtained for two of the variables AE Phe and ε CrA, and a preliminary modelling of the light curves.

Type
II. Photometric Research Programmes
Information
Symposium - International Astronomical Union , Volume 118: Instrumentation and Research Programmes for Small Telescopes , 1986 , pp. 261 - 263
Copyright
Copyright © Reidel 1986 

References

Budding, E. and Najim, N.N. (1980) Astrophys. and Space Sc. 72, 369 CrossRefGoogle Scholar
Sullivan, D.J. and Trodahl, H.J. (1978) Mon. Not. R. Astr. Soc 183, 201 Google Scholar
Trodahl, H.J. and Sullivan, D.J. (1977) Mon. Not. R. Astr. Soc 179, 209 Google Scholar
Trodahl, H.J., Sullivan, D.J. and Gibb, R.G. (1981) Mon. Not. R. astr. Soc 197, 941 CrossRefGoogle Scholar