The CD -247599 Campaign of 1994 (DSN 11)

After the 1992 data of CD-24 7599 had been analysed it was clear, that more pulsation modes than detected must be present. Therefore, the star was re-observed by WET in May, 1994. The number of detectable pulsation frequencies of CD-24~7599 has increased to 13. The 3 dominant modes exhibit amplitude variations with a time scale of one month as well as frequency variations.
7 observatories could acquire data:

Publications following this campaign :