activity
20152022
most citedHR 6819 is a binary system with no black hole -- revisiting the source with infrared interferometry and optical integral field spectroscopy

32 citations · 154 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2022★ 32 cited

HR 6819 is a binary system with no black hole -- revisiting the source with infrared interferometry and optical integral field spectroscopy

A. J. Frost, J. Bodensteiner, Th. Rivinius +16

Two scenarios have been proposed to match the existing observational constraints of the object HR 6819. The system could consist of a close inner B-type giant plus a black hole (BH…

astro-ph.SR2022★ 2 cited

Spectroscopy of the massive interacting binary UU Cassiopeiae

P. Hadrava, M. Cabezas, G. Djurašević +9

Context. The eclipsing close binary UU Cas is an interacting massive double-periodic system with a gainer star partly hidden in an accretion disk. Aims. In order to study the physi…

astro-ph.SR2021★ 1 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.SR2021★ 20 cited

Gem: a hierarchical triple system with an outer Be star

Robert Klement, Petr Hadrava, Thomas Rivinius +17

Time series of spectroscopic, speckle-interferometric, and optical long-baseline-interferometric observations confirm that Gem is a hierarchical triple system. It consists of a…

astro-ph.SR2020★ 12 cited

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.SR2019★ 10 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…