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(1993 Aug. 12) subject: VS observations Visual magnitude estimates by VSOLJ members object YYMMDD(UT) mag code Z And 930811.552 110 Kat DX And 930811.552 <130 Kat EG And 930811.551 73 Kat UU Aql 930811.543 <131 Kat KX Aql 930811.542 <140 Kat V603 Aql 930811.541 116 Kat nova1993 Aql 930811.542 135 Kat AE Aqr 930811.543 116 Kat TT Boo 930811.529 <135 Kat UZ Boo 930811.528 <138 Kat UV Cas 930811.549 109 Kat HT Cas 930811.551 <132 Kat KU Cas 930811.551 <132 Kat V465 Cas 930811.551 69 Kat gamma Cas 930811.550 22 Kat rho Cas 930811.550 47 Kat VV Cep 930811.549 52 Kat delta Cep 930811.549 38 Kat mu Cep 930811.549 45 Kat R CrB 930811.528 60 Kat T CrB 930811.528 104 Kat R Cyg 930811.537 139 Kat U Cyg 930811.537 80 Kat W Cyg 930811.538 61 Kat SS Cyg 930811.539 116 Kat AF Cyg 930811.535 73 Kat BF Cyg 930811.533 112 Kat CH Cyg 930811.536 80 Kat CI Cyg 930811.535 110 Kat DF Cyg 930811.536 124 Kat EM Cyg 930811.534 136 Kat EY Cyg 930811.535 <140 Kat V360 Cyg 930811.540 104 Kat V482 Cyg 930811.535 113 Kat V832 Cyg 930811.538 45 Kat V1329 Cyg 930811.539 131 Kat V1339 Cyg 930811.539 63 Kat V1974 Cyg 930811.537 122 Kat P Cyg 930811.534 48 Kat Q Cyg 930811.539 <135 Kat U Del 930811.546 80 Kat EU Del 930811.547 62 Kat YY Her 930811.530 119 Kat AM Her 930811.530 136 Kat V443 Her 930811.530 118 Kat V795 Her 930811.529 129 Kat alpha Her 930811.530 34 Kat XY Lyr 930811.532 63 Kat AY Lyr 930811.533 <134 Kat EP Lyr 930811.533 102 Kat LL Lyr 930811.532 <134 Kat RS Oph 930811.531 116 Kat V426 Oph 930811.531 125 Kat RU Peg 930811.547 105 Kat EF Peg 930811.547 124 Kat combined IP Peg 930811.548 <122 Kat beta Peg 930811.548 26 Kat R Sct 930811.540 61 Kat V Sge 930811.545 109 Kat RZ Sge 930811.544 <130 Kat SV Sge 930811.541 107 Kat WZ Sge 930811.544 <134 Kat FG Sge 930811.544 112 Kat resolved HM Sge 930811.545 114 Kat WW Vul 930811.546 109 Kat PU Vul 930811.544 115 Kat AS338 930811.542 124 Kat Observer's code: Kat: T. Kato (Kyoto, Japan) instruments: 20L,3F,N * RU Peg at maximum. * V426 Oph is in outburst. * Although the radiant is still low, several observers have reported bright (0 mag or brighter) Perseid meteors, suggesting an already high activity.
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vsnet-adm@kusastro.kyoto-u.ac.jp
