HD 41641: A classical $\delta$ Sct-type pulsator with chemical signatures of an Ap star

TL;DR

This study provides a detailed asteroseismic and spectroscopic analysis of HD 41641, a delta Scuti star exhibiting chemical peculiarities and potential magnetic activity, enhancing understanding of its internal structure and pulsation modes.

Contribution

It combines space-based photometry and high-resolution spectroscopy to identify pulsation frequencies, chemical signatures, and surface features, revealing new insights into delta Scuti stars with Ap-like chemical peculiarities.

Findings

90 pulsation frequencies identified

Dominant mode is a nonradial prograde p-mode with m=+1

Chemical peculiarities suggest magnetic field presence

Abstract

Among the known groups of pulsating stars, $\delta$ Sct stars are one of the least understood. Theoretical models do not predict the oscillation frequencies that observations reveal. Complete asteroseismic studies are necessary to improve these models and better understand the internal structure of these targets. We study the $\delta$ Sct star HD 41641 with the ultimate goal of understanding its oscillation pattern. The target was simultaneously observed by the CoRoT space telescope and the HARPS high-resolution spectrograph. The photometric data set was analyzed with the software package PERIOD04, while FAMIAS was used to analyze the line profile variations. The method of spectrum synthesis was used for spectroscopically determining the fundamental atmospheric parameters and individual chemical abundances. A total of 90 different frequencies was identified and analyzed. An unambiguous identification of the azimuthal order of the surface geometry could only be provided for the dominant p-mode, which was found to be a nonradial prograde mode with m = +1. Using $T_\mathrm{eff}$ and $\log g$, we estimated the mass, radius, and evolutionary stage of HD 41641. We find HD 41641 to be a moderately rotating, slightly evolved $\delta$ Sct star with subsolar overall atmospheric metal content and unexpected chemical peculiarities. HD 41641 is a pure $\delta$ Sct pulsator with p-mode frequencies in the range from 10 d$^{-1}$ to 20 d$^{-1}$. This pulsating star presents chemical signatures of an Ap star and rotational modulation due to surface inhomogeneities, which we consider indirect evidence of the presence of a magnetic field.