activity
20122026
most citedA distance to the Large Magellanic Cloud that is precise to one per cent

686 citations · 2.3k across the 61 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

39 papers · 1 filter

astro-ph.SR2026

Finding the elusive RR Lyrae companions via speckle imaging

R. Salinas, V. Kalari, G. Hajdu +25

Despite their key role in astrophysics, the binary properties of RR Lyrae stars (RRL) remain almost completely unknown since only a single RRL is confirmed as belonging to a binary…

astro-ph.SR2026

Period-Luminosity Relations, projection factor and radii of Anomalous Cepheids

Piotr Wielgórski, Grzegorz Pietrzyński, Wolfgang Gieren +24

Anomalous Cepheids are radially pulsating stars observed in dwarf galaxies, the Galactic bulge and halo, and globular clusters. Similarly to other radially pulsating stars, they ca…

astro-ph.SR2025

Distance to the Globular Cluster M 3 from the Infrared Surface Brightness Technique applied to RR Lyrae stars

Bartłomiej Zgirski, Wolfgang Gieren, Grzegorz Pietrzyński +10

The Infrared Surface Brightness (IRSB) technique is a specific application of the Baade-Wesselink method. Given a proper calibration, well covered optical and near-infrared photome…

astro-ph.SR2025★ 2 cited

Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands

W. Narloch, G. Hajdu, G. Pietrzynski +7

Type II Cepheids (T2Ceps), alongside RR Lyrae stars, serve as important distance indicators for old population II stars due to their period-luminosity (PL) relations. However, stud…

astro-ph.SR2025

Non-evolutionary effects on period change in Magellanic Cepheids II. Empirical constraints on non-linear period changes

Rajeev Singh Rathour, Radosław Smolec, Gergely Hajdu +5

Classical Cepheids are not only excellent standard candles, but also invaluable tools to test stellar evolution and pulsation theories. Rates of their pulsation period change, quan…

astro-ph.SR2025

Non-evolutionary effects on period change in Magellanic Cepheids

R. S. Rathour, R. Smolec, G. Hajdu +5

Classical Cepheids are a cornerstone class of pulsators, fundamental to testing stellar evolution and pulsation theories. Their secular period changes, characterized through …