... (I think I am subscribed to all of these lists, but will restrict any further responses to aavso-discussion only) Sebastian's question is at the crux of...
What kind of dust is it? Where does it come from? How do we account for its longevity; how is it replenished? arXiv:0811.0363 Date: Mon, 3 Nov 2008 18:40:38...
Electronic Telegram No. 1562 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory,...
Electronic Telegram No. 1564 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 18, Smithsonian Astrophysical Observatory,...
I know, you're thinking what in the world does this have to do with cataclysmic variables? Well, read on and I'll explain it to you at the end...I promise. ...
Some of you may have noticed, we have changed the cadence of the distribution of the CVnet Circular to once per week. It should reach your email box every...
Regarding the new Var in Pegasus (OT_J213701.8+071446): As Patrick Wils has already noted [cvnet-discussion 1189], this star was bright on NEAT images taken on...
... The object was also in outburst on 2 Heidelberg plates from 2/3 August 1913 <http://vo.uni-hd.de/lswscans/res/positions/q/form>. Only 6 plates are...
To Variable Star Observers - Southern Hemisphere I have received a request from Brian Warner of the University of Capetown who wishes to be alerted if there is...
Hi all, Since a few weeks I have been following V650 Ori and V392 Per with the Bradford Robotic Telescope. When looking at the AAVSO f-chart (2001) for V650...
On Sat, Dec 6, 2008 at 3:17 PM, Eddy Muyllaert ... The position is correct in VSX and correct using VSP to plot the field. I would suggest that you throw away...
... There is a single outburst to mag 13.1 in NSVS data: <http://www.aavso.org/vsx/docs/25916/22/V392Per.gif>. The data in NSVS near mag 15 are for the...
In what way is it not correct, Hubert? give us a chart ID so that we can see your problem. Remember if you are using the DSS version that stars have proper...
On the chart plotted by Mike Simonsen and a sequence by Henden/Sumner (010123), V650 Ori is identified as the very faint star directly South of that which is...
... Samus supposedly did a painstaking check of GCVS identifications, and came up with the brighter star to the north. Downes and Shara also have this star....
Chartnumber is 1064coy. Hubert. VVS Werkgroep Veranderlijke Sterren http://www.vvs.be/wg/wvs/ ... [Non-text portions of this message have been removed]...
I have analysed photometry conducted by several members of CBA, AAVSO and BAA obtained during the outburst. This includes data from Tom Krajci, Bob Koff, Tut...
I observed IQ Eri last night: It is around mag 12.7, with variations up to 1 mag. May be a 18mn pulsation suggesting an IP but that needs confirmation. Indeed...
D. Denisenko (IKI, Moscow) and S. Korotkiy (Ka-Dar observatory) report: We have observed the Catalina transient OT_J071126.0+440405 [vsnet-alert 10867] with...
From Pauline Loader, RASNZ I am pleased to be able to announce that the RASNZ Council has just approved the appointment of Dr Tom Richards director of the...
This is excellent news; I hope that some standardization in terms of reporting criteria will be developed. Dr. Clay _____ Arkansas Sky Observatories MPC H45 -...
XSS J0056+4548 : a hard X-ray intermediate polar in the period gap ATel #1895; J.M. Bonnet-Bidaud (CEA Saclay), D. de Martino (INAF, Obs Napoli), M. Mouchet...
Had to smile when I saw this one. Mike Title: The HYPERMUCHFUSS Campaign -- an undiscovered high velocity population Authors: Alfred Tillich, Stephan Geier,...
Hi all, Found this on VSNET: http://www.kusastro.kyoto-u.ac.jp/vsnet/circ/ugwait.html This can be very useful to follow our CV's! But what are the different...
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