activity
20142022
most citedDeciphering the 3D structure of the old Galactic bulge from the OGLE RR Lyrae stars

175 citations · 1.4k across the 45 of their papers we have counts for

collaborators

46 papers

astro-ph.GA2022★ 26 cited

A three-dimensional map of the Milky Way using 66,000 Mira variable stars

Patryk Iwanek, Radosław Poleski, Szymon Kozłowski +13

We study the three-dimensional structure of the Milky Way using 65,981 Mira variable stars discovered by the Optical Gravitational Lensing Experiment (OGLE) survey. The spatial dis…

astro-ph.SR2022

New Short-Period Delta Scuti Stars in OGLE-IV Fields toward the Galactic Bulge

P. Pietrukowicz, M. Ratajczak, I. Soszynski +12

We report the classification of 24 puzzling short-period variable stars located in OGLE-IV Galactic bulge fields. The stars are low-amplitude (<0.05 mag) multi-periodic objects wit…

astro-ph.HE2022★ 98 cited

An X-ray quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud

Tomer Shenar, Hugues Sana, Laurent Mahy +35

Stellar-mass black holes are the final remnants of stars born with more than 15 solar masses. Billions are expected to reside in the Local Group, yet only few are known, mostly det…

astro-ph.SR2022★ 6 cited

Precision measurement of a brown dwarf mass in a binary system in the microlensing event OGLE-2019-BLG-0033/MOA-2019-BLG-035

A. Herald, A. Udalski, V. Bozza +89

Context. Brown dwarfs are poorly understood transition objects between stars and planets, with several competing mechanisms having been proposed for their formation. Mass measureme…

astro-ph.SR2021★ 24 cited

Multiwavelength properties of Miras

Patryk Iwanek, Szymon Kozłowski, Mariusz Gromadzki +12

We comprehensively study the variability of Miras in the Large Magellanic Cloud (LMC) by simultaneous analysing light curves in 14 bands in the range of 0.524 microns. We model…

astro-ph.SR2021★ 47 cited

Binarity as the Origin of Long Secondary Periods in Red Giant Stars

I. Soszyński, A. Olechowska, M. Ratajczak +13

Long secondary periods (LSPs), observed in a third of pulsating red giant stars, are the only unexplained type of large-amplitude stellar variability known at this time. Here we sh…