activity
20072021
most citedThe January 2015 outburst of a red nova in M31

36 citations · 71 across the 7 of their papers we have counts for

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Showing astro-ph.SRShow all

14 papers · 1 filter

astro-ph.SR2020

Standing on the shoulders of giants: New mass and distance estimates for Betelgeuse through combined evolutionary, asteroseismic, and hydrodynamical simulations with MESA

Meridith Joyce, Shing-Chi Leung, László Molnár +3

We conduct a rigorous examination of the nearby red supergiant Betelgeuse by drawing on the synthesis of new observational data and three different modeling techniques. Our observa…

astro-ph.SR2019★ 23 cited

Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae Minoris

László Molnár, Meridith Joyce, László Kiss

Most aspects of stellar evolution proceed far too slowly to be directly observable in a single star on human timescales. The thermally pulsing asymptotic giant branch is one except…

astro-ph.SR2018

Wandering near the red edge: photometric observations of three cool ZZ Ceti stars

Zs. Bognár, M. Paparó, Á. Sódor +11

We summarize our findings on three cool ZZ Ceti type pulsating white dwarfs. We determined eight independent modes in HS 0733+4119, of which seven are new findings. For GD 154, we…

astro-ph.SR2018

The s process in AGB stars as constrained by a large sample of Barium stars

B. Cseh, M. Lugaro, V. D'Orazi +8

Context. Barium (Ba) stars are dwarf and giant stars enriched in elements heavier than iron produced by the slow neutron-capture process (s process). They belong to binary systems…

astro-ph.SR2018

All-sky RR Lyrae Stars in the Gaia Data

Lorenzo Rimoldini, Laurent Eyer, Nami Mowlavi +22

The second Gaia data release is expected to contain data products from about 22 months of observation. Based on these data, we aim to provide an advance publication of a full-sky G…

astro-ph.SR2018

Shockwave Behaviour in RR Lyrae Stars

Attila Bódi, László Molnár, Emese Plachy +1

Here we present the detailed analysis of some modulated Kepler and K2 RR Lyrae stars that show peculiar bump progression in respect to the pulsation phase.