1995/12/14 by I. Semeniuk, Semeniuk, I., A. Olech +3
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9512098
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
arxiv created 1995/12/14 · arxiv updated 2009/12/01
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.