Y Cygni

The early type of Y Cyg made it a popular target for astronomers in the past, and spectroscopic orbits have been historically computed numerous times. The first of these studies was published in 1920 by John Stanley Plaskett. Extensive spectroscopic studies of Y Cyg were carried out as early as 1930. Several follow-ups to these have been published in 1959, 1971, and 1980. The latter of these contained an estimate of the period of apsidal precession. ==References==