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