183 UV GEMINORUM (UGSU) Range: 14.2-19.0V Position: 06 38 44.16 +18 16 11.5 (J2000, from .dat file) Magnitude: V=19.041 B-V=0.223 (Henden, single night ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 06 38 58.0 +18 13 18 197 -174 4 11.179 0.250 0.483 0.030 2 06 38 18.4 +18 14 17 -368 -115 1 11.833 0.001 0.706 0.001 3 06 38 50.0 +18 13 17 83 -175 3 12.510 0.039 1.188 0.048 4 06 38 22.9 +18 15 15 -304 -57 3 12.775 0.027 0.385 0.014 5 06 38 26.9 +18 17 21 -246 69 3 13.427 0.028 0.746 0.009 6 06 38 45.5 +18 15 38 18 -34 3 14.129 0.027 0.856 0.009 7 06 38 52.8 +18 17 37 123 85 3 14.419 0.022 0.746 0.008 8 06 38 28.2 +18 16 26 -228 14 3 14.706 0.025 0.566 0.011 9 06 38 43.2 +18 17 04 -14 52 3 15.062 0.032 0.703 0.002 10 06 38 43.4 +18 14 54 -11 -78 3 15.618 0.031 0.746 0.004 11 06 38 46.9 +18 16 58 39 46 3 16.267 0.044 1.164 0.027 12 06 38 49.4 +18 15 45 74 -27 3 17.303 0.049 0.895 0.049 13 06 38 51.0 +18 16 03 97 -9 2 18.242 0.051 1.263 0.018 b) Wide-colour extension for CCD calibration 06 38 53.0 +18 22 06 125 354 3 12.979 0.023 1.806 0.008 06 38 55.9 +18 16 24 167 12 3 12.786 0.020 1.976 0.016 Notes: 1. Stars #1 and #2 are is saturated and their magnitude and colour are approximate. They should be used for guidance only until more accurate values are determined. 2. UV Gem is the eastern component of a faint 19th magnitude double star, with separation about 6 arcsec. Both components are of almost equal magnitude when UV Gem is in quiescence, the variable fairly contant at about V=19.0 in minimum and its companion about V=19.1. 3. There is a preliminary AAVSO(e) chart for this variable with a CCD(V) sequence by Kato, et. al., Kyoto University: Star Henden AAVSO V V 1 11.100 105 3 12.492 122 ext 12.788 126 6 14.135 138 7 14.424 141 9 15.071 146 10 15.628 152 4. Superhumps with a period of 0.0902d were detected during the superoutburst of December 1999 by Vanmunster 1999, vsnet-alert 3821. Bruce Sumner 5 December 2000 Revised 20 January 2001