activity
20192021
most citedOn the long cycle variability of the Algol OGLE-LMC-DPV-065 and its stellar, orbital and disk parameters

10 citations · 26 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20211 cited

Fundamental parameters of the eclipsing binary DD CMa and evidence for mass exchange

J. A. Rosales, R. E. Mennickent, G. Djurašević +5

We present a detailed photometric and spectroscopic analysis of DD CMa, based on published survey photometry and new spectroscopic data. We find an improved orbital period of $P_\m…

astro-ph.SR20215 cited

Stellar and accretion disk parameters of the close binary HD 50526

J. A. Rosales, R. E. Mennickent, G. Djurašević +5

We present a photometric and spectroscopic study of HD 50526, an ellipsoidal binary member of the group Double Periodic Variable stars. Performing data-mining in photometric survey…

astro-ph.SR2020

New insights on the massive interacting binary UU Cassiopeiae

R. E. Mennickent, G. Djurašević, I. Vince +7

We present the results of the study of the close binary UU Cassiopeiae based on previously published multi wavelength photometric and spectroscopic data. Based on eclipse timings o…

astro-ph.SR20207 cited

Long photometric cycle and disk evolution in the Lyrae type binary OGLE-BLG-ECL-157529

R. E. Mennickent, J. Garcés, G. Djurašević +4

The subtype of hot algol semidetached binaries dubbed Double Periodic Variables (DPVs) are characterized by a photometric cycle longer than the orbital one, whose nature has been r…

astro-ph.SR201910 cited

On the long cycle variability of the Algol OGLE-LMC-DPV-065 and its stellar, orbital and disk parameters

R. E. Mennickent, M. Cabezas, G. Djurašević +13

OGLE-LMC-DPV-065 is an interacting binary whose double-hump long photometric cycle remains hitherto unexplained. We analyze photometric time series available in archive datasets sp…

astro-ph.SR20193 cited

Long-term Spot Stability in the Post-common-envelope Binary QS Vir

Olivera Latković, Attila Cséki, Gojko Djurašević +3

We observed the post-common-envelope eclipsing binary with a white dwarf component, QS Vir, using the 1.88 m telescope of Kotammia Observatory in Egypt. The new observations were a…