CCD Photometry of Nova V1500 Cygni Twenty Years After

Details CCD Photometry of Nova V1500 Cygni Twenty Years After CCD Photometry of Nova V1500 Cygni Twenty Years After

1995-12-14

arxiv.org/abs/astro-ph/9512098v1

Astronomy and Astrophysics

Astrophysics

accepted for publication in Acta Astronomica, 6 pages, compressed PostScript with one figure included; also available through

Scientific paper

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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