Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Astronomical Observatory, Volgina 7, 11050 Belgrade, Yugoslavia
Astronomical Observatory, Isaac Newton Institute of Chile, Yugoslav Branch, Volgina 7, 11160 Belgrade, Serbia and Montenegro
Astronomical Observatory, Volgina 7, 11160 Belgrade 74, Serbia
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia and Montenegro and Isaac Newton Institute of Chile, Yugoslav branch, Yugoslavia
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia
Beograd, Astronomska Opservatorija, Belgrade, Yugoslavia
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, 11000 Belgrade, Serbia
Astronomical Observatory of Belgrade
Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Volgina 7, 11060 Belgrade 38, Serbia
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia and Montenegro ; Isaac Newton Institute of Chile, Yugoslav branch
Astronomical Observatory, Volgina 7, 11160 Belgrade, Yugoslavia and Isaac Newton Institute of Chile, Yugoslav branch
Astronomical Observatory of Belgrade, Volgina 7, 11060 Belgrade 38, Serbia
Astronomical Observatory, Volgina 7, YU-11050 Belgrade, Yugoslavia
Astronomical Observatory; Isaac Newton Institute of Chile, Yugoslav Branch
Astronomical Observatory, Belgrade, Yugoslavia Newton Institute of Chile, Yugoslav Branch, Santiago, Chile
Astronomical Observatory, Volgina 7, 11160 Belgrade, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Volgina 7, 11160 Belgrade, Serbia
Astronomical Observatory
Astronomical Observatory, Belgrade, Yogoslavia
Astronomical Observatory, Belgrade, Yugoslavia
Astronomical Obser
2001-2003 BV differential photometry of SW Lac (Albayrak+, 2004)
4 close binaries BVR light curves (Djurasevic+, 2011)
A light and period study of SV Camelopardalis
A model of light-curve synthesizing for dwarf novae and the analysis of the OY CAR observations by application of the inverse-problem method
A photometric study of eclipsing binary V351 Pegasi
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