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Issue A&A
Volume 397, Number 3, January III 2003
Page(s) 951 - 959
Section Stellar atmospheres
DOI http://dx.doi.org/10.1051/0004-6361:20021539



A&A 397, 951-959 (2003)
DOI: 10.1051/0004-6361:20021539

Modelling the recurrent nova CI Aql in quiescence

C. Lederle and S. Kimeswenger

Institut 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 $\dot M \approx 2.5 \times 10^{-8}\,\,{M}_\odot\,{\rm
yr}^{-1}$ in 1991-1996 to $5.5 \times 10^{-8} < \dot M < 1.5
\times 10^{-7}\,\,{M}_\odot\,{\rm yr}^{-1}$ in 2001/2002. The distance and the interstellar foreground extinction resulting from the model are 1.55 kpc and $E_{B-V} = 0\fm98$ respectively. During fast photometry sequences in 2002 short timescale variations ( $t_{\rm F} \approx 13$ 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 $2.2
\times 10^{-6} < \Delta M < 5.7 \times 10^{-6}\,\,{M}_\odot$ 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

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