Long-term cycles in old Novae

Details Long-term cycles in old Novae Long-term cycles in old Novae

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..985s&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Nov. 1989, p. 985-990.

Astronomy and Astrophysics

Astronomy

16

Astronomical Photometry, Charge Coupled Devices, Novae, Secular Variations, Stellar Evolution, Variable Stars

Scientific paper

Three of the oldest recovered novae were monitored with a CCD camera almost nightly for six weeks. The cyclic variability reported by Della Valle and Rosino (1987) for Nova Oph 1848 is confirmed. A similar variability is also suggested for Nova Cyg 1876, though this system exhibits more random flickering than Nova Oph. No secular variability is seen in Nova Sge 1783.

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