Another interesting new cataclysmic variable, EN Cet. Excerpt from IAUC 6763: CATACLYSMIC VARIABLE IN CETUS The Beijing Astronomical Observatory (BAO) supernova survey, with A. Esamdin, Urumqi Astronomical Station, reports their discovery on Oct. 28, using the 0.6-m reflector at Xinglong Station, of a cataclysmic variable star in outburst at R.A. = 0h27m27s.93, Decl. = -1 08'26".8 (equinox 2000.0). Available R magnitudes: Oct. 17.64 UT, 14.5; 21.67, 14.9; 28.61, 15.4; 29.61, 15.6; 30.45, 15.8. The variable did not apppear on CCD images obtained on Oct. 8 (limiting mag 18.5), and it appears as a very faint object on the original Palomar Sky Survey. A spectrum of the star, obtained by X. Dong and Y. Zhao with the BAO 2.16-m telescope at Xinglong on Oct. 30.56, shows typical features of cataclysmic variables in outburst, with mainly a blue continnum at 500-800 nm, and a spectrum at 380- 500 nm that is similar to the dwarf nova CY Lyr at maximum, with absorption of H-delta, H-gamma, H-beta, and weak He I (447.1 nm). Charts with a preliminary visual sequence from USNO A2.0 are now online at http://joevp.20m.com/charts/sxncharts/Cet%20EN%20Rsxn.gif and http://joevp.20m.com/charts/sxncharts/Cet%20EN%20sxn.gif Regards, Mike Simonsen