We report on CCD photometry of Nova V1500 Cygni obtained in July 1995 to show that twenty years after outburst, being of about 18mag, the star can still be observed with small telescopes. The 0.1396 day period continues to be stable.
- Pub Date:
- October 1995
- STARS: INDIVIDUAL: V 1500 CYG;
- BINARIES: CLOSE;
- NOVAE: CATACLYSMIC VARIABLES;
- accepted for publication in Acta Astronomica, 6 pages, compressed PostScript with one figure included