(1993 Jan. 3)
subject: T Leo
Dear Gary,
Thanks to your timely alert, I have already started high speed
CCD photometry of this interesting object and followed a full orbital
cycle. The observation is still continuing. The magnitude can not
be told directly from the TV monitor, but is much brighter than than
nearby 11.9 mag (GSC) star.
I am looking forward to seeing the coming data from Europe this
night.
Regards,
Taichi Kato

Return to the Powerful Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp