Abbott, T.M.C.; Shafter, A.W.; Wood, J.H.; Tomaney, A.B. and Haswell, Carole
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Photometric and spectroscopic observations of DO Leo have been obtained using the McDonald Observatory high-speed CCD photometer and a conventional two-channel photoelectric photometer. The data reveal eclipses that are approximately 1.5 m deep. A total of nine eclipses were observed in February and March 1988 and in April 1989. These data were used to establish an orbital period of 0.2345147(2) d. A low-resolution optical spectrum reveals significant He II 4686 emission in addition to the characteristic Balmer and He I emission lines.
|Item Type:||Journal Article|
|Keywords:||Astronomical photometry; cataclysmic variables; eclipsing binary stars; novae; orbit calculation; stellar orbits; electrophotometry; sky brightness; stellar spectra|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Astrid Peterkin|
|Date Deposited:||01 Aug 2008 14:40|
|Last Modified:||04 Oct 2016 14:57|
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