The chemical composition of the Herbig Ae SB2 system AK Sco (HD152404)

TL;DR

This study analyzes the chemical composition of the Herbig Ae SB2 system AK Sco, revealing element abundances and peculiarities, and comparing them to typical Herbig Ae/Be star patterns using high-resolution spectra.

Contribution

First detailed abundance analysis of AK Sco's components, identifying elemental peculiarities and comparing them to known Herbig star patterns.

Findings

Identified elements typical of F5IV-V stars, with Li I and He I related to Herbig nature.

Found overabundances of Y, Ba, La in both stars.

Zirconium overabundant only in the primary, sulfur only in the secondary.

Abstract

We investigate the stellar atmospheres of the two components of the Herbig Ae SB2 system AK Sco to determine the elements present in the stars and their abundance. Equal stellar parameters T_eff = 6500K and log g = 4.5 were used for both stars. We studied HARPSpol spectra (resolution 110,000) that were previously used to state the presence of a weak magnetic field in the secondary. A composite synthetic spectrum was compared in the whole observed region lambda 3900-6912A with the observed spectrum. The abundances were derived mostly from unblended profiles, in spite of their sparsity, owing to the complexity of the system and to the not negligible v sin i of 18km/s and 21km/s adopted for the two components, respectively. The identified elements are those typical of stars with spectral type F5IV-V, except for Li I at 6707A and He I at 5875.61A, whose presence is related with the Herbig nature of the two stars. Furthermore, overabundances were determined in both stars for Y, Ba, and La. Zirconium is overabundant only in the primary, while sulfur is overabundant outside the adopted error limits only in the secondary. In contrast to previous results showing a high occurrence rate of lambda Boo peculiarities or normal chemical composition among the Herbig Ae/Be stars, the abundance pattern of AK Sco is similar to that of only few other Herbig stars displaying weak Ap/Bp peculiarities. A few accretion diagnostic lines are discussed.