From jop at astro.columbia.edu Mon Sep 14 19:38:10 2020 From: jop at astro.columbia.edu (Joe Patterson) Date: Mon, 14 Sep 2020 19:38:10 -0400 Subject: (cba:news) Fwd: (cba:chat) The Return of Maxie?... and some expired "suoersoft" stars In-Reply-To: References: Message-ID: <06100de7-a8a2-8ceb-2a55-ac415d144ad3@astro.columbia.edu> Thanks Joe for this important notification. Maxie has (ASASSN-18ey)still not reached its expiration date. Long time series are no longer possible, but a 1-hour observation is just fine. Our regular-journal paper is nearing completion. One last outburst of any size would be a fitting send-off. We also have finished with V617 Sgr, QR And, and CI Aql... which are bundled in with the paper on IM Nor and T Pyx. All these stars are done for the year. Around 15 of you, who have observed these stars, will be getting the first version of this very detailed paper shortly. The main issue that the IM Nor et al. paper addresses is this: how much does a classical-nova event affect the basic structure of the binary, and how long does that disturbance persist? (And the suggested answers are surprising: a lot, and for centuries, possibly millennia). Sure has been fun writing it! September-October menu coming in a day or so. joe -------- Forwarded Message -------- Subject: (cba:chat) The Return of Maxie? Date: Mon, 14 Sep 2020 18:08:37 -0500 From: Joe Ulowetz Reply-To: cba-chat at cbastro.org To: cba-chat at cbastro.org If ASASSN-18ey (Maxie) follows the pattern from the past couple of years, I expect another outburst sometime within the next few weeks.? I got some data last night through the West Coast smoke (and I'm in Chicago), and my data looks like mag 16.1 which is about 2 magnitudes brighter. Of course, this is a really tentative measurement but I should be able to check again tonight. If you've been following Maxie as well, I encourage you to check as well to see if the next outburst has started. Thanks, -Joe U. -------------- next part -------------- ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/ -------------- next part -------------- ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/ From jop at astro.columbia.edu Wed Sep 23 14:44:21 2020 From: jop at astro.columbia.edu (Joe Patterson) Date: Wed, 23 Sep 2020 14:44:21 -0400 Subject: (cba:news) Sep-Oct-Nov stars Message-ID: <8aed0ef0-c259-6128-fa0e-8b6239c11566@astro.columbia.edu> Hi CBAers, New stars for the new season. I'll separate into northern and southern. As usual, it's a good idea with one or two favorite targets. (If there's gold in any of these stars, I'll send up a signal!) But inevitably all Earthly campaigns have gaps, and if they're too big, then period studies become uncertain NORTH V392 Per. Make this recent nova high priority. So far, the star shows a pretty good 1.1 hour signal - a puzzler. But on a few good nights, it's missing - so that's suspicious. Since it's far northern and the observing season is just starting, we should be able to do very well on it. Mag 15.0 now. V378 Peg. We have some good data from past years - seemingly orbit + superhump. 2020 will nail everything down. V1500 Cyg and BY Cam. "Asynchronous polars". The general idea here is: orbital period stable and known, spin period unstable on some timescale, which isn't really known. Not so hard to measure, though - you just need to construct an O-C curve WITHOUT MISCOUNTING CYCLES. But that can be challenging if the orbital signal is not quite of known amplitude and phase. So a really good job is needed - hence the desirablity of "crowd-sourcing". V1500 might be quite faint. V598 Peg. A nice well-placed IP, and time for us to mount a big campaign. SOUTH CC Scl - A mighty interesting IP, one of the few at short Porb. Let's mount a strong campaign. AH Men - we haven't written anything on this guy since 1995, and have lots of data ready to roll if we can get one more season. ES Cet - let's extend that the long-term study of timing. Finally, one subject area I would really like to stress is ORBITAL LIGHT CURVES OF OLD NOVAE. Old just meaning a few (or more) years after the nova eruption. None strike me as being particularly seasonal right now, but you might find some that are well-placed and within your magnitude limit. V959 Mon is a definite possibility, but still maybe too early in the season... AAVSO virtual meeting coming up in November - abstracts due Sep 30, I think. joe ____________________________________________________________ Center for Backyard Astrophysics (CBA) mailing lists https://cbastro.org/communications/mailing-lists/