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).

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