The 1982 standstill of HL CMa

(vsnet-obs 4216)

Patrick Schmeer wrote (vsnet-obs 4179):

> Is HL CMa a UGZ or UGSS dwarf nova?

Examination of the AFOEV and VSOLJ light curves (1982-now) shows only one standstill in 1982 April. HL CMa may be a Z Cam star having a low frequency of standstills.

Regards,
Taichi Kato

Light curve based on the AFOEV and VSOLJ observations

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