activity
20242026
collaborators

6 papers

astro-ph.GA2026

Reddening maps of the Magellanic Clouds using spectral energy distribution fitting of red giants

H. Netzel, G. Pietrzyński, M. Górski +9

Robust reddening maps of the Large and Small Magellanic Clouds (LMC/SMC) are crucial for a wide range of astrophysical studies, including the calibration of the cosmic distance lad…

astro-ph.SR2026

Reconstruction of Cepheid Radial Velocity Curves from the shape of the V-band Light Curves

V. Hocdé, P. Moskalik, N. Nardetto +17

This paper aims to develop the first method to reconstruct the shape of the RV curves of short-period fundamental-mode Cepheids, based exclusively on their pulsation period and the…

astro-ph.SR2025

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

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

astro-ph.SR2025

Toward early-type eclipsing binaries as extragalactic milestones: IV. Physical properties of three detached O/B-type systems in the LMC

Mónica Taormina, G. Pietrzyński, R. -P. Kudritzki +10

We present a complete set of physical parameters for three early-type eclipsing binary systems in the Large Magellanic Cloud (LMC): OGLE LMC-ECL-17660, OGLE LMC-ECL-18794, and HV 2…

astro-ph.SR2024

Circumstellar emission of Cepheids across the instability strip: Mid-infrared observations with VLTI/MATISSE

V. Hocdé, A. Matter, N. Nardetto +14

The circumstellar envelopes (CSE) of Cepheids are still not well characterized despite their potential impact on distance determination via both the period-luminosity relation and…