Visual observations of outbursts Rod Stubbings (VSS-RASNZ) Drouin, Vic. Australia. Instrument: 32cm Newtonian Star Date UT Mag. --------------------------------------- CN ORI 990506 9:04 <13.3 990510 8:46 12.9 HL CMA 990506 9:14 <13.7 990510 8:50 11.6 YZ CNC 990506 8:59 <14.0 990510 8:53 12.1 X LEO 990506 9:34 <14.8 990510 9:10 12.5 BX PUP 990506 9:18 <14.4 990510 9:25 14.3 CU VEL 990508 12:46 <14.6 990510 9:35 10.9 Current outbursts, V1159 ORI 990510 8:47 13.7 AT CNC 990510 9:00 13.0 VW HYI 990510 9:11 8.9 BV PUP 990510 9:24 13.8 UY PUP 990510 9:28 14.3 V442 CEN 990510 9:44 14.7 V436 CEN 990510 9:45 13.5 IK NOR 990510 10:12 13.6 BF ARA 990510 12:03 14.3 TU IND 990510 12:53 13.9 FO AQL 990510 15:21 14.4 Observations, CZ ORI 990510 8:45 <13.8 SY CNC 990510 9:03 12.8 ST CHA 990510 9:17 14.4 EP CAR 990510 9:18 15.3 V651 MON 990510 9:30 11.4 V803 CEN 990510 9:43 <15.2 V834 CEN 990510 9:58 15.0 NV MUS 1998 990510 10:06 14.4 SGRV4444 990508 14:37 10.8 seq:Henden SGRV4444 990510 12:19 10.9 seq: Henden 1432-0033 990510 10:42 15.0 * 1432-0033 990510 15:15 15.0 * * Re: 1432-0033 This field was observed for the first time using the VSNET chart. According to the chart, there is no star of this brightness near the possible variable. Time will tell if the possible variable brightens, remains or fades.