most citedA theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC

4 citations · 9 across the 6 of their papers we have counts for

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astro-ph.SR20253 cited

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.SR20252 cited

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…

astro-ph.SR20244 cited

A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC

Susmita Das, László Molnár, Gábor B. Kovács +8

We carry out an extensive light curve comparison of BL Her stars using observations from Gaia DR3 and stellar pulsation models computed using MESA-RSP with the goal to obtain the b…

astro-ph.SR20241 cited

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.SR2024

Validation of the RR Lyrae period determination in the Pan-STARRS PS1 3 survey with K2

Adrienn Forró, László Molnár, Emese Plachy +2

The Pan-STARRS 3 survey has detected hundreds of thousands of variable stars thanks to its coverage and 4-year time span, even though the sampling of the light curves is relativ…