CCD Photometry of Nova V1500 Cygni Twenty Years After
I. Semeniuk, A. Olech, M. Nalezyty
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.
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