CCD Photometry of Nova V1500 Cygni Twenty Years After

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dc.creatorSemeniuk, I.
dc.creatorOlech, A.
dc.creatorNalezyty, M.
dc.date1995-12-14
dc.date.accessioned2026-07-07T02:20:37Z
dc.date.available2026-07-07T02:20:37Z
dc.descriptionWe 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.
dc.descriptionaccepted 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9512098
dc.identifierhttp://arxiv.org/abs/astro-ph/9512098
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10267
dc.subjectAstrophysics
dc.titleCCD Photometry of Nova V1500 Cygni Twenty Years After
dc.typetext

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