18 citations · 29 across the 8 of their papers we have counts for
10 papers
rapidsim: A Python interface and cross-platform distribution framework for the RAPID protoplanetary disc simulation code
D. Tarczay-Nehéz
The rapidsim is a Python package for the RAPID (Representative Approach for Particle-Integrated Disks) numerical simulation code, which is a modular one-dimensional hydrodynamic si…
A blue-straggler merger scenario origin for the ~Persei binary system
D. Tarczay-Nehéz, L. Molnár, R. Z. Ádám
We used \texttt{MIST} isochrone fitting and a dedicated grid of stellar evolution models computed with MESA to constrain the ages of the components of the Persei binary system.…
Trajectory-Based Dust Evolution in Disks: First Results from the RAPID Simulation Code
D. Tarczay-Nehéz
The rapid depletion of dust particles in protoplanetary disks limits the time available for planetesimal formation, as solids are typically accreted onto the central star before du…
Stranger Things: A Grid-based Survey of Strange Modes in Post-Main Sequence Models
D. Tarczay-Nehéz, L. Molnár, M. Joyce
We present a systematic survey of strange mode pulsations in Cepheids using MESA and for the linear stability analysis, MESA RSP. Our model grid spans in mass and […
MESAlab: A Python pipeline for MESA grid processing with integrated GYRE/MESA-RSP execution
D. Tarczay-Nehéz
Modules for Experiments in Stellar Astrophysics (MESA) is a widely used open-source code for modeling stellar evolution. Many applications of the code rely on large computational g…
Stellar Evolution in Real Time II: R Hydrae and an Open-Source Grid of >3000 Seismic TP-AGB Models Computed with MESA
Meridith Joyce, László Molnár, Giulia Cinquegrana +3
We present a comprehensive characterization of the evolved thermally pulsing asymptotic giant branch (TP-AGB) star R Hydrae, building on the techniques applied in Stellar Evolution…
Testing ultralow amplitude Cepheid candidates in the Galactic disk by TESS and Gaia
Dóra Tarczay-Nehéz, László Molnár, Attila Bódi +1
Ultralow amplitude (ULA) and strange mode Cepheids are thought to be pulsating variable stars that are near to or are at the edges of the classical instability strip. Until now, a…
Planetary nurseries: vortices formed at smooth viscosity transition
Zs. Regaly, K. Kadam, D. Tarczay-Nehez
Excitation of Rossby wave instability and development of a large-scale vortex at the outer dead zone edge of protoplanetary discs is one of the leading theories that explains horse…
Variable star classification with a Multiple-Input Neural Network
T. Szklenár, A. Bódi, D. Tarczay-Nehéz +3
In this experiment, we created a Multiple-Input Neural Network, consisting of Convolutional and Multi-layer Neural Networks. With this setup the selected highest-performing neural…
On the evolution of vortex in locally isothermal self-gravitating discs: a parameter study
D. Tarczay-Nehéz, K. Rozgonyi, Zs. Regály
Gas rich dusty circumstellar discs observed around young stellar objects are believed to be the birthplace of planets and planetary systems. Recent observations revealed that large…