activity
20062023
most citedAsteroseismology of old open clusters with Kepler: direct estimate of the integrated RGB mass loss in NGC6791 and NGC6819

348 citations · 1.4k across the 16 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2023★ 18 cited

Calibration of the convective parameters in stellar pulsation hydrocodes

Gábor B. Kovács, Róbert Szabó, János Nuspl

Despite the appearance of two- and three-dimensional models thanks to the rapid growth of computing performance, numerical hydrocodes used to model radial stellar pulsations still…

astro-ph.SR2019★ 125 cited

The first view of Scuti and Doradus stars with the TESS mission

V. Antoci, M. S. Cunha, D. M. Bowman +63

We present the first asteroseismic results for Scuti and Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…

astro-ph.SR2018★ 4 cited

unVEil the darknesS of The gAlactic buLgE (VESTALE)

G. Bono, M. Dall'Ora, M. Fabrizio +55

The main aim of this experiment is to provide a complete census of old (t > 10 Gyr, RR Lyrae, type II Cepheids, red horizontal branch), intermediate age (red clump, Miras) and youn…

astro-ph.SR2014★ 66 cited

Looking for activity cycles in late-type Kepler stars using time-frequency analysis

K. Vida, K. Oláh, R. Szabó

We analyse light curves covering four years of 39 fast-rotating () late-type active stars from the Kepler database. Using time-frequency analysis (Short-Term Fo…

astro-ph.SR2012★ 6 cited

New results in RR Lyrae modeling: convective cycles, additional modes and more

L. Molnár, Z. Kolláth, R. Szabó +1

Recent theoretical and observational findings breathed new life into the field of RR Lyrae stars. The ever more precise and complete measurements of the space asteroseismology miss…

astro-ph.SR2012★ 61 cited

Period and light curve fluctuations of the Kepler Cepheid V1154 Cyg

A. Derekas, Gy. M. Szabo, L. Berdnikov +11

We present a detailed period analysis of the bright Cepheid-type variable star V1154 Cygni (V =9.1 mag, P~4.9 d) based on almost 600 days of continuous observations by the Kepler s…