From jop at astro.columbia.edu Sat Aug 5 04:50:36 2006 From: jop at astro.columbia.edu (Joe Patterson) Date: Sat, 05 Aug 2006 04:50:36 -0400 Subject: (cba:news) august stars Message-ID: <44D45BDC.3060304@astro.columbia.edu> Dear CBAers, We've gone to a new computer system here at Columbia, and some mail may have gotten lost from down time, overenthusiastic spam blockers, etc. So please bear with us, and re-send anything critical. Two new Sagittarius stars on the menu. V1830 Sgr has jumped into (super)outburst, and is a high-priority target for as long as it stays bright. There are no published time series of this star - or unpublished either, for that matter. Secondly, our analysis of June-July CBA coverage of V1223 Sgr has suggested a superhump signal in that star, which would be awfully important if true (because it would demonstrate that tidal instability is not inhibited by magnetic fields). But our data is not sufficiently extensive to clinch the point - we need a couple of weeks coverage from all our strong southern nodes (ZA, NZ, AU) and perhaps something from the southern USA too. I think there's still time in this observing season to carry out this study. Sooo... despite my previous removal of this star from the menu, couldja put it back - with high priority? The star is about 14th mag and has an obvious 13 minute pulse as well as a possible 3.6 hr superhump signal; pretty nice target! And it's now time to turn northern telescopes on V Sge, an old CBA favorite which we have neglected for about a decade. This would be a fine target for the bright of the Moon, which seems appropriate now. The main interest is timing the (sometimes subtle) eclipse. This star is very luminous and quite rapidly evolving; the eclipses will yield the RATE of evolution, and this will go far to clarify the nature of this class of star (more or less the supersoft binaries). The other all-hemisphere star I wanted to press for is V1494 Aql, which is very well placed now if you can get this faint (about 16) with a bright moon lurking nearby. One additional season to yield its 3-hour orbital light curve (which changes year-to-year as the star cools from the 1999 nova eruption) will complete our study with superb coverage every year! I'll write again when I find out whether this even goes out... maybe 50-50 with the new system - and my inexperience with using it! joe From jop at astro.columbia.edu Sat Aug 12 05:05:27 2006 From: jop at astro.columbia.edu (Joe Patterson) Date: Sat, 12 Aug 2006 05:05:27 -0400 Subject: (cba:news) DQ Her etc. In-Reply-To: References: <44D45BDC.3060304@astro.columbia.edu> Message-ID: <44DD99D7.9040808@astro.columbia.edu> Hi Lew and others, Yes, I think it's time to drop DQ Her... unless you can manage 15 second time resolution with 40:1 signal to noise. That's roughly what it takes to capture the 71 s signal. The coverage so far takes care of the eclipses. The bright moon makes V Sge a particularly good northern choice these days, with AO Psc a good follow-on. The menu will get a little more ambitious when the Moon gets more docile next week. Enjoy the Perseids! joe