A study of the stellar photosphere-hydrogen ionization front interaction in $\delta$ Scuti stars

TL;DR

This study examines the interaction between the hydrogen ionization front and the stellar photosphere in $\

Contribution

It provides the first observational analysis of PCAC relations in $\

Findings

Observed PCAC relations support HIF-photosphere interaction theory

Analysis includes stars from Galactic bulge and LMC

Uses MESA-RSP code for modeling

Abstract

Pulsating variable $\delta$ Scuti stars are intermediate-mass stars with masses in the range of $1-3$ $M_{\odot}$ and spectral types between $A2$ and $F2$. They can be found at the intersection of the Cepheid instability strip with the main sequence. They can be used as astrophysical laboratories to test theories of stellar evolution and pulsation. In this contribution, we investigate the observed period-colour and amplitude-colour (PCAC) relations at maximum/mean/minimum light of Galactic bulge and Large Magellanic Cloud $\delta$ Scuti stars for the first time and test the hydrogen ionization front (HIF)-photosphere interaction theory using the MESA- RSP code. The PCAC relations, as a function of pulsation phase, are crucial probes of the structure of the outer stellar envelope and provide insight into the physics of stellar pulsation and evolution. The observed behaviour of the $\delta$ Scuti PCAC relations is consistent with the theory of the interaction between the HIF and the stellar photosphere.