A. Bianchini
Abstract
Analyse statistique des courbes de lumiere a long terme des vieilles novae GK Per, Q Cyg et V841 Oph, du systeme type nova TT Ari et des 2 systemes prototypes de nova naine SS Cyg et U Gem qui a revele l'existence de cycle d'activite stellaire de periode 6,9, 6,6, 3,3, 12,6, 7,3 et 6,9 ans, respectivement
OpenAlex reports 2 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Analyse statistique des courbes de lumiere a long terme des vieilles novae GK Per, Q Cyg et V841 Oph, du systeme type nova TT Ari et des 2 systemes prototypes de nova naine SS Cyg et U Gem qui a revele l'existence de cycle d'activite stellaire de periode 6,9, 6,6, 3,3, 12,6, 7,3 et 6,9 ans, respectivement
Key concepts: Nova (rocket), Dwarf nova, Cataclysmic variable star, Astrophysics, Physics, Humanities, Art, White dwarf