ECLIPSING DWARF NOVAE PROGRAMME UPDATE MAY 2007 ROGER PICKARD I’m grateful to Bill Worraker for providing the following update to this programme. There are now only 13 stars left on this programme and it would be nice if observers (both visual and CCD) could supply some concentrated coverage to see if any of these stars are eclipsing dwarf novae. Below are notes on current programme stars. Those to be dropped from now on are marked: AR And 4.0 hours photometry received to date, no sign of eclipses. FO And 1.68 hours photometry (Thorstensen et al 1996), no eclipses. KV And 3 orbits covered (Kato et al 1994), no eclipses > DROP TT Boo Many orbits covered (Olech et al 2004), no eclipses > DROP AT Cnc 1orbit + 2 part orbits covered (Nogami et al 1999), no eclipses (also deduced to have low inclination.) > DROP CC Cnc Many orbits covered (Kato et al 2002), no eclipses > DROP GX Cas 3-4 orbits covered (Nogami et al 1998, Nick James), no eclipses > DROP KU Cas No data (not even an orbital period), published or unpublished. SV CMi No photometry. V516 Cyg 4.1 hrs photometry (Nick James), no eclipses. V1060 Cyg No data, published or unpublished. ES Dra 1.5 orbits (Misselt+Shafter 1995), 1.4+1.6 orbits (CBA Belgium 2001). No eclipses, but flickering noted - keep on programme as outburst behaviour is uncertain and P_orb has been revised downward to approximately 3 hours (type SU UMa?) AW Gem 4 orbits covered (Kato 1996), no eclipses > DROP SX LMi Many orbits covered (Nogami et al 1997, Wagner et al 1998), no eclipses/low inclination > DROP CY Lyr Bits of photometry (0.6+0.4 orbits), no eclipses. LL Lyr No photometry. V344 Lyr 4 orbits covered (Kato et al 1993), no eclipses > DROP V426 Oph 0.9+0.75orbits covered (Hollander et al 1993); no eclipses (inclination 59+/-6 deg, Hessman 1988), but a strange object which deserves some attention. HX Peg No photometry. TZ Per 0.9+0.8 orbits covered (Nick James; Mumford 1966), no eclipses > DROP PY Per No photometry; CI UMa 4 orbits covered (Nogami+Kato 1997), no eclipses > DROP HS Vir Some orbital photometry (Kato et al 1998), no eclipses -> DROP VW Vul Some orbital photometry (Kato 1999), no eclipses > DROP FY Vul No data, published or unpublished. The Programme therefore becomes: Object Name Coordinates Type Min Max T1 P_orb(h) Altern.Name (J2000) T2 P_shu(h) ----------------------------------------------------------------------------- AR And 01 45 03.27 UG? 16.9 11.0 25 3.91(DS2) +37 56 33.3 FO And 01 15 32.1 SU 17.5 13.5 15-23 1.7186 +37 37 36 1.779 KU Cas 01 31 02.6 UG 18p 13.3p ?? ?? (DS) +57 54 12.3 SV CMi 07 31 08.5 ZC 16.3 13 16 3.74 + 05 58 47 V516 Cyg 20 47 09.9 UG 16.8p 13.8p ?? ?? (DS) +41 55 26 V1060 Cyg 21 7 42.3 UG 18p 13.5p ?? ?? (DS) +37 14 08.3 ES Dra (DS2) 15 25 31.8 DN? 16.3p 13.9p ?? 4.238 PG 1524+622 +62 1 00.1 CY Lyr 18 52 41.41 UG? 17.0 13.2 ?? 3.82 (DS2) +26 45 29.9 LL Lyr 18 35 12.91 UG? 17.1 12.8 ?? ?? (DS2) +38 20 04.3 V426 Oph 18 7 51.8 ZC 13.4 11.5 17-55 6.847 +05 51 48 HX Peg 23 40 23.8 ZC 16.6 12.0 9 4.819 PG 2337+123 +12 37 41 PY Per 02 50 00.2 ZC 19.8 13.0 8 3.715 +37 39 22 FY Vul 19 41 40 ZC 15.3B 13.4B ?? ?? (DS) +21 45 59 Symbols: DS Data taken from Downes and Shara, PASP 105, 127 (1993) DS2 Data taken from Downes, Webbink and Shara, PASP 109, 345 (1997) p photographic magnitude T1 Normal outburst interval (days) T2 Superoutburst interval (days) DN Dwarf Nova UG Dwarf Nova, U Gem type ZC Dwarf Nova, Z Cam type SU Dwarf Nova, SU UMa type