activity
20042026
most citedA distance to the Large Magellanic Cloud that is precise to one per cent

686 citations · 1k across the 33 of their papers we have counts for

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astro-ph.SR20251 cited

Empirical instability strip for classical Cepheids II. The Small Magellanic Cloud galaxy

Felipe Espinoza-Arancibia, Bogumił Pilecki, Matylda Łukaszewicz

Aims. This study aims to determine empirical intrinsic edges of the classical Cepheids instability strip (IS) in the Small Magellanic Cloud (SMC) galaxy, considering various effect…

astro-ph.SR2025

The nature of ASASSN-24fw's occultation: modelling the event as dimming by optically thick rings around a sub-stellar companion

Sarang Shah, Jonathan P. Marshall, Carlos del Burgo +12

ASASSN-24fw is a main-sequence F-type star that experienced a rapid and long-lasting dimming event beginning in late 2024 and continuing until mid 2025. Its pre-dimming spectral en…

astro-ph.SR2025

A novel q-PED method: precise physical properties of a merger-origin binary Cepheid OGLE-LMC-CEP-1347

Felipe Espinoza-Arancibia, Bogumił Pilecki

Recently, a double-lined binary (SB2) classical Cepheid, OGLE-LMC-CEP-1347, was discovered, with the orbital period (P days) five times shorter than of any binary…

astro-ph.SR2025

Cepheids in spectroscopic binary systems -- current status and recent discoveries

Bogumił Pilecki

We present a summary of the current knowledge about Cepheids in binary systems. We focus on the most recent findings and discoveries, such as the highly increasing number of confir…

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…