FYI, for our southern Hemisphere observers. Mike Simonsen American Association of Variable Star Observers http://aavso.org/ C. E. Scovil Observatory ...
This enigmatic variable has been classified and re-classified several times in the last few years. I think it is generally agreed now that DW Cnc is an...
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Boris.Gaensicke@...
Jan 29, 2007 1:28 pm
Dear All, DW Cnc is a very puzzling object... ... Looking at its (relatively sparse) long term light curve, V~14.5 is its typical brightness, but it has shown...
Hi All, Now that five papers on CVs in the Sloan Digital Sky Survey (SDSS) are publicly available, I thought it was time to evaluate these discoveries to ...
... - Electronic Telegram No. 834 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory,...
Confirm presence of new object. Astrometry with UCAC2 data (15 reference stars) gives the following: (11-inch SCT, f.l.=2850mm) UT date of obs, YYYY MM DD:...
... This astrometric result probably has less *accuracy* than quoted above. Unfortunately, -32 Dec is quite low in New Mexico, and Tom was observing ...
Magnitude is based on UCAC2/CR data. ... Tom Krajci Cloudcroft, New Mexico http://overton2.tamu.edu/aset/krajci/ Center for Backyard Astrophysics (CBA) ...
SDSS163605.01+465204.5 Feb 7.247 15.4C This is the first time I have observed this star so I am not sure what it's normal mag is, although I note in Mike...
Hello Jeremy, Looking at DSS images there are indeed two stars of similar brightness with a separation about 3". The CV is the western one. In infrared it is...
... Under poor conditions I measured it at v = 9.47 +/- 0.04 at Feb. 7 11:20 UT (JD 54138.97), using ASAS V = 9.54 for TYC 7364-1358-1. Using Tycho B-V for...
Further to Arne's note (below), I have drawn up a chart and sequence that extends the current BAAVSS sequence from 13.1V to 16.3V. My comparisons are overlaid ...
... -- ... -- The Astronomer's Telegram http://www.astronomerstelegram.org ... -- Posted: Fri Feb 23 01:30:01 EST 2007 -- Sat Feb 24 01:30:03 EST 2007 ...
We are going into our third year of full contact cataclysmic variable activity, discussion, sharing and reporting on CVnet. I'd like to take a moment to thank...
Thanks Boris. So it could be UGSU then? You will have seen that I detected a brightness variation - pity I wasn't able to do a longer run. Interested observers...
SS Aur certainly is in outburst, but I found it very difficult to visually evaluate using the 110 and 109 comp stars on the 3-08-25 AAVSO chart. The star...
Neither star is red, in fact they are both fairly blue, so color shouldn't be a factor. 109 is definitely brighter, but not by very much. I'd probably use the...
Yup, 11.0, not 10.0. ... From: cvnet-discussion@yahoogroups.com [mailto:cvnet-discussion@yahoogroups.com] On Behalf Of Mike Simonsen Sent: Wednesday, March 14,...
To my utmost frustration, I had a Bradford Robotic Telescope job completed on PQ And a day before Eddie's announcement - and the field was just off frame!...
SN2007af appears to be one of the brightest SN in quite some time. I have seen several reports in the 12th magnitude range as recently as March 17 UT. It...
Another apparent nova. This one in Ophiuchus. ************************************************************ Electronic Telegram No. 900 Central Bureau for...
Recently published in "Peremennye Zvezdy", Prilozhenie, vol. 7, N 8 (2007), the author uses ASAS data and 2MASS colors to determine NSV 6052 is a UGSS. It...
Recently published in "Peremennye Zvezdy", Prilozhenie, vol. 7, N 8 (2007), the author uses ASAS data and 2MASS colors to determine NSV 6052 is a UGSS. It...
I'm looking for images of DV Dra in outburst (last one was November 2005) to settle an identity question that keeps popping up on the AAVSO charts. FITS, GIF,...
Hi Mike, I have 53 images taken Nov. 25, 2005. Since they are all 518 Kb, there is no way my "slowdem' will get them all out to you. I can compress the fits...
