Unveiling the variability and chemical composition of AL Col

Abstract

In this study, we present analysis of TESS photometry, spectral energy distribution (SED),high-resolution spectroscopy, and spot modeling of the α 2 CVn-type star AL Col (HD 46462). The primary objective is to determine its fundamental physical parameters and investigate its surface activity characteristics. Using TESS short-cadence (120 s) SAP flux, we identified a rotational frequency of 0.09655 d −1(Prot = 10.35733 d). Wavelet analysis reveals that while the amplitudes of the harmonic components vary over time, the strength of the primary rotational frequency remains stable. A SED analysis of multi-band photometric data yields an effective temperature (Teff) of 11,750 K. High-resolution spectroscopic observations covering wavelengthrange 4500–7000 Å provide refined estimates of Teff = 13,814 ± 400 K, log g = 4.09 ± 0.08 dex, and υ sin i = 16 ± 1 km s−1. Abundance analysis shows solar-like composition of O II, Mg II, S II, and Ca II, while helium is under-abundant by 0.62 dex. Rare earth elements (REEs) exhibit over-abundances of up to 5.2 dex, classifying the star as an Ap/Bp-type star. AL Col has a radius of R = 3.74 ± 0.48R⊙, with its H–R diagram position estimating a mass of M = 4.2 ± 0.2M⊙ and an age of 0.12 ± 0.01 Gyr, indicating that the star has slightly evolved from the main sequence. The TESS light curves were modeled using a three-evolving-spot configuration, suggesting the presence of differential rotation. This star is a promising candidate for future investigations of magnetic field diagnostics and the vertical stratification of chemical elements in its atmosphere.