This star is a VERY large amplitude TOAD and suspected of being a magnetic system. The chart in Downes and Shara, has the exact star misid'ed, however, at outburst, there will be no doubt of its location as there are no other bright stars nearby. AL Com had its last outburst in 1975 (last known) and is HIGHLY likely to have a post outburst brigntening. So do not stop observations after it fades, watch for a rebrightening a day or so later, upto about 14th or so. The minimum magnitude ofr AL Com is near 20.5 and in previous outbursts it got as bright as 12th or so. Superhump observations as well as spectra (no previous ones exist) would be very useful. Further information can be obtained from the undersigned good observing. Steve Steve B. Howell Planetary Science Institute, Astrophysics Group 620 N. 6th Ave. Tucson, AZ 85705 USA Phone (520) 622-6300 Fax (520) 622-8060 e-mail: howell@frankenstein.psi.edu homepage: http://vsnet.psi.edu/