During this tutorial, we shall try and find the preliminary solution of the UV Leonis
binary system. UV Leonis
is a detached close binary with coordinates
and
. Data files for this system are acompanying every PHOEBE release and reside in data/UVLeo
directory. There are two photometric light curves3 in B and V filters (both from Bessel 1990 series): UVLeo.B
and UVLeo.V
and two radial velocity curves4: UVLeo.rv1
and UVLeo.rv2
- one for each star.