CCD Photometry of Nova V1500 Cygni Twenty Years After
arXiv:astro-ph/9512098
Abstract
We report on CCD photometry of Nova V1500 Cygni obtained in July 1995 to show that twenty years after outburst, being of about 18~mag, the star can still be observed with small telescopes. The 0.1396 day period continues to be stable.
accepted for publication in Acta Astronomica, 6 pages, compressed PostScript with one figure included; also available through WWW at http://www.astrouw.edu.pl/~olech/v1500.html