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20212026
most citedTemperature dependent convective parameters for RRc 1D-models

11 citations · 17 across the 8 of their papers we have counts for

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8 papers

astro-ph.SR2026

Asteroseismic Analysis of the Merger Product Red Giant in the Persei System

Rozália Z. Ádám, László Molnár, Róbert Szabó +7

Context. Persei is a long-period eclipsing binary system ( years) containing a red giant primary, and it is well known for its multi-faceted classification as a…

astro-ph.EP2025

Three fast-spinning medium-sized Hilda asteroids uncovered by TESS

Nóra Takács, Csaba Kiss, Róbert Szakáts +8

Hilda asteroids, which orbit in a 3:2 resonance with Jupiter, serve as key indicators of dynamical processes in the early solar system. Their spin rates, an important probe of thes…

astro-ph.SR2025★ 4 cited

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

Gabriella Zsidi, Ágnes Kóspál, Péter Ábrahám +20

Classical T Tauri stars are newly formed, low mass stars which may display both periodic and random variations in their brightness. The interaction between the star and its circums…

astro-ph.SR2025★ 2 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.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…

astro-ph.SR2024

On the use of field RR Lyrae as Galactic probes VII. light curve templates in the LSST photometric system

V. F. Braga, M. Monelli, M. Dall'Ora +5

The \textit{Vera C. Rubin} Observatory will start operations in 2025. During the first two years, too few visits per target per band will be available, meaning that mean magnitude…

astro-ph.SR2023★ 11 cited

Temperature dependent convective parameters for RRc 1D-models

Gábor B. Kovács, János Nuspl, Róbert Szabó

Nonlinear pulsation modeling of classical variable stars is among the first topics which were developed at the beginning of the computational era. Various developments were made, a…

astro-ph.SR2021

Ancillary science with Ariel: Feasibility and scientific potential of young stellar object observations

Boldizsár I. Gyűrűs, Csaba Kiss, Juan Carlos Morales +7

To investigate the feasibility of ancillary target observations with ESA's Ariel mission, we compiled a list of potentially interesting young stars: FUors, systems harbouring extre…