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[vsnet-obs 2973] (fwd) Re: Fading of V705 Cas
- Date: Mon, 17 Jun 1996 16:29:49 +0900
- To: vsnet-obs
- From: Taichi Kato <tkato>
- Subject: [vsnet-obs 2973] (fwd) Re: Fading of V705 Cas
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Date: Mon, 17 Jun 1996 01:15:56 +0100
From: gp@star.sr.bham.ac.uk (Gary Poyner)
To: SDI00707@niftyserve.or.jp
Dear all,
In response to Reinder Bouma's note re. V705 Cas.
I too have been puzzled by observations of V705 Cas posted to VSNET
over the past few weeks or so, except that I have found it strange
that some observers were reporting it so faint!
I can state with every confidence that the object which I have been monitoring
is NOT GSC 4008.1363. I have been observing this nova since
discovery in 1993 (300+ observations), and am absolutely confident that I
am estimating the nova's brightness and not a field star. Both the TA and
AAVSO charts identify the same object, which rules out any ID problem.
I have just made an observation of V705 Cas, taking great care (as usual)
with the estimate. Although slightly fainter than last night, I still
make it brighter than my Dutch friends. The observation is...
Jun 16.993 16-2 12.7 Class 1 40cm Seq. TA
(Star 18 on the TA seq.(133 AAVSO) looks a little bright to me)
I take it that the magnitude of GSC 4008.1363 noted by Reinder in his message
(approx. 12.5) was a combined one, as this star is obviously a
double.
Regards,
Gary Poyner