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My research has been related mostly to the problem of the angular momentum evolution in binary stars, from the stage of formation to their coalescence. I also worked some time ago on the interstellar polarization, star formation, proto-stellar disks and stellar atmospheres, but most of my work currently is related to binary stars, especially contact binary stars. The last, larger project done at the David Dunlap Observatory using the DDO 1.88m telescope was a systematic spectroscopic survey of bright close binary stars with periods shorter than 1 day. I developed the Broadening Function approach for the DDO spectroscopic data and for similar uses; it gives far superior results to the Cross-Correlation Function. The MOST satellite project ended its long and profitable life and I am now very involved in another satellite project BRITE which was also started in Canada. I was the early leader of the Canadian team of the BRITE Canadian Team (see a PDF description) and am now a member of the international committee overseeing BRITE Constellation operations.
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ASTRONOMICAL JOURNALno. 3 (2020)
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