[vsnet-alert 13819] BW Scl : ordinary superhump transition

[Ohshima]

BW Scl : ordinary superhump transition

 We have received further observations from Maehara-san, Kiyota-
san, Itoh,san, and Microlensing Observations in Astrophysics
Group.
 As to the past mail by Kato-san, the ordinary superhumps have
been developing. Despite of shortness observations after the
transition, 0.0555 (5) d is obtained as the ordinary superhump
period. This implies that the superhump excess is 2.1 %.

 Further observations are strongly encouraged!