Long-Term Photometry of Very Slow Novae

Abstract: Long-term photographic, photoelectric and recent CCD photometry of the classical nova V723 Cas and symbiotic novae V1329 Cyg, PU Vul, V1016 Cyg and HM Sge were used to find their orbital periods. The arguments in favor of the presence of the third components in these systems are given. Physical processes, responsible for the brightness variations, are discussed.

Location
Deutsche Nationalbibliothek Frankfurt am Main
Extent
Online-Ressource
Language
Englisch

Bibliographic citation
Long-Term Photometry of Very Slow Novae ; volume:12 ; number:4 ; year:2003 ; pages:610-615 ; extent:6
Open astronomy ; 12, Heft 4 (2003), 610-615 (gesamt 6)

Creator
Chochol, D.
Pribulla, T.
Parimucha, Š.
Vaňko, M.

DOI
10.1515/astro-2017-0089
URN
urn:nbn:de:101:1-2405271635595.645101660201
Rights
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
Last update
14.08.2025, 10:50 AM CEST

Data provider

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Associated

  • Chochol, D.
  • Pribulla, T.
  • Parimucha, Š.
  • Vaňko, M.

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