collaborators

8 papers

astro-ph.SR2025

New theoretical instability regions, period-luminosity relations and masses for blue large-amplitude pulsators

Susmita Das, Daniel Jadlovský, László Molnár

Blue large-amplitude pulsators (BLAPs) are a recently discovered group of hot pulsating stars whose evolutionary status remains uncertain. Their supposed progenitors are either $\s…

astro-ph.SR2025

Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4

László Molnár, Henryka Netzel, Madeline Howell +2

Globular clusters offer a powerful way to test the properties of stellar populations and the late stages of low-mass stellar evolution. In this paper we study oscillating giant sta…

astro-ph.SR2025

Connections between the cycle-to-cycle light curve and O-C variations of the non-Blazhko RR Lyrae stars

J. M. Benkő, A. Bódi, E. Plachy +1

It has long been known that if the durations of the consecutive cycles of a pulsating star vary randomly, the O-C diagram could show quasi-periodic/irregular variations, even thoug…

astro-ph.SR2025

Search for binary-channel metal-rich RR~Lyrae candidates

Hedieh Abdollahi, László Molnár, Vázsony Varga

The existence of dynamically young and metal-rich RR Lyrae stars challenges conventional notions of these variable stars. One possible scenario for their formation and evolution is…

astro-ph.EP2025

Three fast-rotating Jovian Trojans identified by TESS set new population density limits

Csaba Kiss, Nóra Takács, Csilla E. Kalup +8

Here we report on the identification of the three fastest rotating Jovian Trojans with reliable population assignment, using light curve data from the Transiting Exoplanet Satellit…

astro-ph.SR2025

A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters

Susmita Das, László Molnár, Róbert Szabó +5

We present new theoretical light curves in the Rubin-LSST filters for a fine grid of BL Her models computed using MESA-RSP. We also derive new theoretical period-luminosity (PL) an…