TW Pic
A. Pearce reported that the intermediate polar or permanent superhumper
TW Pic showed a fading to <15.3 on January 2.767. The observation may
be somewhat contradicting with B. Monard's observation of 14.9 on January
2.806d. TW Pic is also suggested as a possible VY Scl-type system
(Norton et al. 2000, MNRAS 312, 362)
(vsnet-campaign 651).
A. Pearce's observation showed it became slightly brighter (14.7mag)
on January 4
(vsnet-campaign 655).