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Scientific Highlights:

2017 - JunPeculiar W Vir type Cepheid mass determination First determination of the mass and the projection factor for the Cepheid OGLE-LMC-T2CEP-098 in a binary system.
2017 - AprOccurrence of BEPs Simulations of Binary Evolution Pulsators predict their occurrence in the instability strip of RR Lyrae and Cepheid variables
2016 - OctLL Aqr LL Aqr
2015 - DecMass determination for classical FU Cepheid Precise mass determination for a classical Cepheid in the double-lined, highly eccentric eclipsing binary system OGLE-LMC562.05.9009
2015 - SepCarina distance Carina distance determined from infrared period-luminosity relation of RR Lyrae stars.
2015 - JunFirst-overtone Cepheid mass determination First determination of the mass and the projection factor for the first-overtone Cepheid OGLE-LMC-CEP-2532 in a binary system.
2014 - MayBinary system of two Cepheids Binary system OGLE-LMC-CEP-1718 composed of two classical FO Cepheids confirmed spectroscopically and analized.
2014 - JanSMC distance SMC distance determined with the accuracy of 3% using binary systems composed of giants.
2013 - DecFirst dynamical p-factor determination First determination of the projection factor from the analysis of eclipsing binary systems for the Cepheid OGLE-LMC-CEP-0227 together with very precise physical parameters.
2013 - MarLMC distance LMC distance determined with the accuracy of 2% using binary systems composed of giants.
2012 - AprBinary Evolution Pulsator (BEP) New type of RR Lyrae-like variable identified in a binary system.
2011 - DecDynamical mass of a Cepheid (CEP-1812) Very precise mass determination of the Cepheid OGLE-LMC-CEP-1812 in an eclipsing binary system.
2010 - NovDynamical mass of a Cepheid (CEP-0227) Very precise mass determination of the Cepheid OGLE-LMC-CEP-0227 in an eclipsing binary system.