-
BVRcIC photometry of V2615 Oph
The moderately fast Nova Oph 2007 reached maximum brightness on 2007 March 28 at V=8.52, B-V=+1.12, V-Rc=+0.76, V-Ic=+1.59 and Rc-Ic=+0.83 , after fast initial rise and a... -
R light curve of DO Dra
We study the variability of the cataclysmic variable DO Dra, on time-scales of between minutes and decades. The observations were obtained at the Korean 1m telescope at the Mt.... -
IPHAS symbiotic stars candidates
The study of symbiotic stars is essential to understand important aspects of stellar evolution in interacting binaries. Their observed population in the Galaxy is however poorly... -
Stroemgren photometry of Dwarf Novae
A sample of 26 dwarf novae was observed in the Stroemgren photometric system. The observations were performed on 3 different seasons in 1986 January, February and July, with a... -
VBLUW Observations of TT Ari
TT Ari was observed in the 5 passbands VBLUW (544, 430, 384, 362 and 324nm) during 3 nights on the 90cm telescope at ESO (La Silla), between July and November 1988, with an... -
Walraven photometry of WX Hyi
The SU UMa-type dwarf nova WX Hyi was observed in the 5 passbands VBLUW (544, 430, 384, 362 and 324nm) during 15 nights on the 90cm telescope at ESO (La Silla), between July and... -
Cataclysmic Binaries, LMXBs, and related objects
(no description available) Cone search capability for table B/cb/cbdata (Catalogue of Cataclysmic Binaries) Cone search capability for table B/cb/lmxbdata (Catalogue of Low-Mass...
