New nova in delphinus
#1
Posted 14 August 2013 - 04:21 PM
http://www.cbat.eps....73 2046041.html
Just visualy observed it and estimated it 6.5. AAVSO chart 12506UL
Compstars 62 and 70.
Easy visible in 8x42 bino.
#2
Posted 14 August 2013 - 04:24 PM
#3
Posted 14 August 2013 - 08:55 PM
Very nice and easy to find.
#4
Posted 14 August 2013 - 09:19 PM
#5
Posted 14 August 2013 - 11:45 PM
GOT IT!!!!! Topocentric vs J2000 issue.
#6
Posted 15 August 2013 - 01:18 AM
Taras
#7
Posted 15 August 2013 - 02:07 AM
Joe
#8
Posted 15 August 2013 - 03:14 AM
#9
Posted 15 August 2013 - 05:00 AM
Rich (RLTYS)
#10
Posted 15 August 2013 - 05:52 AM
Cheers -
Rob
#11
Posted 15 August 2013 - 07:17 AM
#12
Posted 15 August 2013 - 10:10 AM
I would note that it is a rare thing to actually view a nova when precisely at maximum, most of them being discovered some days (sometimes weeks) after they have peaked and they are fading.
It will prove interesting to see just what type of nova this new object will be, fast, normal, or slow. HR Del 1967 was situated about 10 degrees to the SE of the new nova's position. It was a very slow nova, remaining near maximum for a couple of months! However, its rise to maximum was much slower and its amplitude less than seems to be the case with the new object.
BrooksObs
#13
Posted 15 August 2013 - 10:49 AM
I found a link with a good pdf chart
http://www.freestarc...s/186-bright...
#14
Posted 15 August 2013 - 10:54 AM
#15
Posted 15 August 2013 - 12:02 PM
#17
Posted 15 August 2013 - 02:38 PM
Dean
#18
Posted 15 August 2013 - 03:24 PM
BrooksObs
#19
Posted 15 August 2013 - 04:29 PM
#20
Posted 15 August 2013 - 04:35 PM
PNV J20233073+2046041 20130815.858 4.77R 0.04 4 CMC
-Juanjo
#21
Posted 15 August 2013 - 04:37 PM
That is 1.4 magnitude brighter in 24 hours. Keep on watching it!
#23
Posted 15 August 2013 - 04:49 PM
Thanks for the chart Hubert - very helpful.
#24
Posted 15 August 2013 - 06:35 PM
www.flickr.com/photos/79652716@N00/9518001289/lightbox/
Keith.
#25
Posted 15 August 2013 - 08:36 PM
Lexington, KY USA 9:36 pm edst








