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A&A 397, 951-959 (2003)
DOI: 10.1051/0004-6361:20021539
Modelling the recurrent nova CI Aql in quiescence
C. Lederle and S. KimeswengerInstitut für Astrophysik der Leopold-Franzens-Universität Innsbruck, Technikerstr. 25, 6020 Innsbruck, Austria
(Received 16 August 2002 / Accepted 30 September 2002)
Abstract
We present detailed photometric investigations of the
recurrent nova CI Aql. New data obtained after the 2000 outburst
are used to derive a 3D geometrical model of the system. The
resulting light curves clearly indicate the existence of an
asymmetric spray around the accretion disk, as claimed in the past
e.g. for the super-soft X-ray source CAL87 in the LMC. The
simulated light curves give us the mass transfer rates varying
from
in 1991-1996 to
in 2001/2002. The
distance and the interstellar foreground extinction resulting from
the model are 1.55 kpc and
respectively. During fast photometry sequences in 2002 short
timescale variations (
min) of the mass
loss are found. Moreover a change in the orbital period of the
system is detectable and results in a mass loss of
during the nova explosion.
Key words: stars: individual: CI Aql -- stars: novae, cataclysmic variables -- accretion, accretion disks -- binaries: eclipsing
Offprint request: S. Kimeswenger, stefan.kimeswenger@uibk.ac.at
SIMBAD Objects
© ESO 2003
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