Cambridge University Press, Proceedings of the International Astronomical Union, S290(8), p. 339-340, 2012
DOI: 10.1017/s1743921312020303
Full text: Unavailable
AbstractWe summarise the results of observing faint cataclysmic variables from the Catalina Real-Time Transient Survey, resulting in confirming the theoretically predicted maximum in the orbital period histogram near a period of 80 minutes.