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[vsnet-obs 5673] Correction
- Date: Sat, 3 May 1997 03:53:58 +0200 (MET DST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp (VSNET observers)
- From: Rudolf Novak <rudolfn@physics.muni.cz>
- Subject: [vsnet-obs 5673] Correction
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Dear readers,
I would like to explain my last mail to vsnet-obs. I've read e-mail from
P. Schmeer in the afternoon and of course forgot name of star till evening
and
was too lazy to check my mbox again. So I observed DY UMa instead CY
UMa. So! DY is in quiescence near to 15.0 therefore I have about two
hours of CCD R-band photometry of this star in quiescence.
To mail about V 391 Lyr. I made 120 sec exposures and using Downes &
Shara's identification can say that the star is not visible (a little bit
is)
but another star close to its position is near 15 mag as reported in
mentioned report.
Please exuse me - I sleep just a few hours a day... :-)
With best regards
Rudolf Novak
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* Rudolf Novak Private: Rudolf Novak *
* Nicholas Copernicus Observatory Bohuslava Martinu 50 *
* Kravi Hora 2 BRNO 602 00 *
* BRNO 616 00 Czech Republic *
* Czech Republic *
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* e-mail: rudolfn@physics.muni.cz *
* h-page: http://vsnet.sci.muni.cz/~rudolfn *
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* " ... no, There's no dark side of the Moon ... " *
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