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[vsnet-campaign-nova 353] Possible Nova Sco 2001, photometry and spectroscopy by Liller
Possible Nova Sco 2001, photometry and spectroscopy by Liller
Date: Thu, 21 Jun 2001 00:44:45 -0400
From: "W.Liller" <wliller@compuserve.com>
Subject: Haseda's nova-like variable
Hola, Everyone -
At UT June 21.660, using nearby GSC 7382 837 as a standard and adopting
V = 9.87, B-V = +0.44, I measured Haseda's nova-like variable with a CCD
to have a broadband V magnitude of 10.68 +/- 0.03. A low dispersion
objective prism spectrogram recorded with the CCD shows a very intense
red line, presumably H-alpha (but remember V445 Pup !), that is approximately
5 times the brightness of the surrounding continuum. H-beta (?) is weakly
present indicating that the star is substantially reddened.
Congratulations Haseda-sen for his discovery ! Cheers,
Bill Liller
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
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