Hubble COS Spectroscopy of the Dwarf Nova CW Mon: The White Dwarf in Quiescence?
Connor Hause et al 2017 AJ 154 48
Synthetic spectral analysis of the HST COS spectrum of the U Geminorum-type dwarf nova CW Mon indicate the presence of a 22–27,000 K WD and a low mass accretion rate.