599 citations · 1.4k across the 42 of their papers we have counts for
42 papers
Beyond MESA Defaults: The Impact of Structural Resolution Uncertainty in p-mode Asteroseismology
Yaguang Li, Meridith Joyce
Observations of pressure modes (-modes) in stars have enabled profound insights into stellar properties, and theoretical stellar evolution and oscillation models are integral to…
Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay Between Mixing Length, Metallicity and
Yaguang Li, Timothy R. Bedding, Daniel Huber +8
Asteroseismic modelling is a powerful way to derive stellar properties. However, the derived quantities are limited by built-in assumptions used in stellar models. This work presen…
A theoretical framework for BL Her stars -- II. New period-luminosity relations in the Gaia passbands
Susmita Das, László Molnár, Shashi M. Kanbur +6
We present new theoretical period-luminosity (PL) and period-Wesenheit (PW) relations for a fine grid of convective BL Her, the shortest period T2Cs, models computed using MESA-RSP…
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…
Detailed asteroseismic modeling of RR Lyrae stars with non-radial modes
H. Netzel, L. Molnar, M. Joyce
Photometric observations from the last decade have revealed additional low-amplitude periodicities in many classical pulsators that are likely due to pulsations in non-radial modes…
Bridging the Gap between Intermediate and Massive Stars II: for the most metal-rich stars and implications for Fe CCSNe rates
Giulia C. Cinquegrana, Meridith Joyce, Amanda I. Karakas
The minimum initial mass required for a star to explode as an Fe core collapse supernova, typically denoted , is an important quantity in stellar evolution because it…