Modelling RRLs using MESA-RSP

The project involves computing stellar pulsation models of RR Lyraes using the state-of-the-art 1D non-linear radial pulsation tool of MESA (Paxton et al. 2019). The aim is to test the effect of convection parameters on the theoretical multi-wavelength period-luminosity relations of RR Lyraes. We estimate ~4000 RRL models per convection set, ushering in an era of large number statistics in the field of stellar modelling. This project is a part of the Élvonal grant (www.konkoly.hu/seismolab/)

Publikációk

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2024

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; Radoslaw Smolec; Meridith Joyce; Shashi M. Kanbur; Tamás Szklenár; Anupam Bhardwaj; Harinder P. Singh; Marcella Marconi et al.
Modelling RRLs using MESA-RSP
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