From jop at astro.columbia.edu Tue Nov 1 11:41:25 2016 From: jop at astro.columbia.edu (Joe Patterson) Date: Tue, 1 Nov 2016 11:41:25 -0400 Subject: (cba:news) Fwd: CC Scl in outburst In-Reply-To: References: Message-ID: Hi CBAers, Very attractive target for southern observers! joe -------- Forwarded Message -------- Subject: CC Scl in outburst Date: Tue, 1 Nov 2016 15:39:47 +0000 From: Gordon Myers To: 'Joe Patterson' , 'Enrique de Miguel' Joe and Enrique, CC Scl went into outburst overnight. You may want to alert the observers ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/ From jop at astro.columbia.edu Fri Nov 4 18:42:49 2016 From: jop at astro.columbia.edu (Joe Patterson) Date: Fri, 4 Nov 2016 18:42:49 -0400 Subject: (cba:news) Fwd: [vsnet-alert 20316] ASASSN-16me: new eclipsing polar In-Reply-To: <581CFDE8.3080909@alumni.nd.edu> References: <581CFDE8.3080909@alumni.nd.edu> Message-ID: Hi CBAers, Here's an exciting report. Eclipsing polars are rare... and let's jump on this one hard, before western twilight clobbers the star. joe -------- Forwarded Message -------- Subject: [vsnet-alert 20316] ASASSN-16me: new eclipsing polar Date: Fri, 4 Nov 2016 17:30:16 -0400 From: Colin Littlefield To: vsnet-alert at ooruri.kusastro.kyoto-u.ac.jp I observed ASASSN-16me on November 4 for approximately 3 hours. Although there are numerous gaps in the time series because of sporadic cloud cover, there is a deep and extremely abrupt eclipse which lasts for 7 minutes, during which the system became undetectably faint. Immediately before and after the eclipse, the system was at mag. ~17.3 (CV bandpass), but during the eclipse, it faded below mag. 19. There is also a very prominent orbital hump which almost certainly results from the changing visibility of the accretion region across the orbital period. Because there are numerous gaps in the light curve, I cannot determine the orbital period based on this data, but I suspect that it is less than 2 hours. I will attempt another time series tonight to find the orbital period. Best Wishes, Colin Littlefield ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/ From edmiguel63 at gmail.com Wed Nov 16 20:33:30 2016 From: edmiguel63 at gmail.com (Enrique de Miguel) Date: Thu, 17 Nov 2016 02:33:30 +0100 Subject: (cba:news) stars for november Message-ID: <1E8E9831-C34E-4F3B-9883-435DD42AE9D6@gmail.com> Dear all, It's time to update our menu. Joe is going through some vision problems and has asked me to take care of the November menu. Well, here it goes, along with suggestions for removing some of our previous targets. TARGETS TO BE REMOVED: ** RX And, ** V592 Cas (only positive superhumps this season), ** V Sge, LQ Peg, and LS Peg. ** BW Scl and AQ Men in the Southern skies. STARS FOR NOVEMBER ** HS 0455+8315 High priority. A new eclipsing, negative superhumper. In addition to the signal associated with the superhump modulation, some of these targets show an additional signal (~4 days) which is believed to be a direct sign of the nodal precession of the accretion disk. For this target, this signal is expected at ~3.6 days, and my bet is that it's there. But we can only proof this if we follow the star along several nodal cycles. ~2 weeks of extensive coverage will tell. At this stage, only long runs are valuable. ** HS 0229+8016 A bright, alleged ZCam star, with brightness variations between ~13.8 and ~15.0 mag. Low-amplitude modulation of orbital nature (Porb ~ 3.88 hr). But in 2014 a short campaign showed another signal, possibly, a superhump. An intensive coverage ~1-2 week coverage should give us a clue. As HS 0455+8315, the target is well placed in Northern skies for all-night runs. For these 2 targets, runs from both sides of the Atlantic would help. ** Intermediate polars (IPs) Good time to get a few early-season runs on the following IPs: V1062 Tau, PQ Gem, V405 Aur, BG CMi and V667 Pup. MU Cam is also a good choice, but Jou U. has done a good job, and we have now a good spin ephemeris that goes back to 2002. We can leave this target for a few weeks and resume coverage by the end of December. We also need a few late-season runs on the "summer" IPs, mainly, AO Psc, V515 And, and V1033 Cas. V647 Aur is slightly more demanding (it needs long runs). And more demanding IPs are V902 Mon, eclipsing, equatorial IP; and Swift J0614.0+1709, a ~17-mag IP, but very rewarding. Some additional (Southern) targets: ** CC Scl Good target. ** HZ Pup. This is a faint (~17.0) intermediate polar (Pspin ~ 20.2 min). Not an easy target, but feasible for some of you in the morning sky. Great target if you can manage to get at least 2-3 h runs. ** T Pyx ~3 h runs now early in the season will be useful to keep track of the orbital signal ** ES Cet A ~17.0 mag AM CVn star, with a fast orbital period (10.3 min) beautifully increasing with time. Berto and Gordon got some runs early in the season. No need of dense coverage -just a few sporadic runs to keep track of the orbital signal. Regards, Enrique ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/