BVRI photometry of extremely slow nova Aql = V1548 Aql

Details BVRI photometry of extremely slow nova Aql = V1548 Aql BVRI photometry of extremely slow nova Aql = V1548 Aql

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..319p&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3

Other

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Photometric, Polarimetric, And Spectroscopic Instrumentation, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays, Hertzsprung-Russell, Color-Magnitude, And Color-Color Diagrams

Scientific paper

The preliminary result of the detail VRI photometry of Nova Aql 2001 = V1548 Aql during the outburst decline is presented. Nova shows an extremely slow fading with rate of 0.006 mag/day over first 150 days. Quasi-regular brightening with typical time ~ 60 days and amplitude up to 1m were superposed on the outburst decline. A peculiarities of behaviour of this nova on the color-color diagram are discussed.

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