activity
20142026
most citedBlack Hole, Neutron Star and White Dwarf Candidates from Microlensing with OGLE-III

155 citations · 886 across the 49 of their papers we have counts for

collaborators

51 papers

astro-ph.SR2026

Highly bipolar planetary nebula Hen 2-57 and its possible symbiotic core

J. Merc, J. Mikołajewska, K. Iłkiewicz +1

We present a multi-wavelength analysis of the highly bipolar object Hen 2-57 based on new optical spectroscopy from the Southern African Large Telescope (SALT), complemented by arc…

astro-ph.SR2025

X-ray properties of RR Lyrae and Cepheid variables from eROSITA

Krystian Ilkiewicz, Henryka Netzel

We present a search for X-ray counterparts to RR Lyrae and Cepheid variables using data from the first eROSITA all-sky survey. We identify seven RR Lyrae and eight Cepheid variable…

astro-ph.SR2025

Identification of new Galactic symbiotic stars with SALT -- II. New discoveries and characterization of the sample

J. Merc, J. Mikołajewska, K. Iłkiewicz +2

We present the continuation of a systematic search for new southern Galactic symbiotic stars, selecting candidates from the SuperCOSMOS H Survey and 2MASS. Follow-up spectroscop…

astro-ph.SR2025

Blending-induced beating and emission in the symbiotic star Terz V 2513

J. Merc, J. Mikołajewska, C. Gałan +4

We present a detailed analysis of Terz V 2513 (=2MASS J17334728-2719266), a poorly studied symbiotic star. Our motivation was a peculiar beating pattern in its light curves from al…

astro-ph.HE2025

Optical and cm follow-ups of the Changing-Look event in Mkn 590

Biswaraj Palit, Abhijeet Borkar, Agata Różańska +5

The Changing-Look active galactic nucleus Mkn 590 is currently in a rejuvenated state, exhibiting a contemporaneous flux rise across X-rays, UV, optical and cm wavelengths. In this…

astro-ph.SR2025★ 1 cited

Circumbinary disc interactions and stochastic dust obscuration in the post-asymptotic-giant-branch binary HD 213985

Krystian Ilkiewicz, Lea Planquart, Tomek Kaminski +1

HD 213985 is an eccentric binary system with a post-AGB primary and a jet-launching secondary star. We confirm that the system photometric variability is likely due to obscuration…