Differential abundance analysis of Procyon and Theta Sculptoris: Comparison with abundance patterns of solar-like pairs

Abstract

The precision differential abundance (PDA) technique is applied to the mid-F stars Procyon and $\theta$ Scl using spectra from the ESO UVESPOP library. We relate PDA patterns to endogenous processes related to condensation or to exogenous processes connected to Galactic chemical evolution (GCE). We employ one-dimensional LTE models, but emphasize the use of weaker lines ($\le$ 20 mÅ) than are typically used in such studies. We compare our results with PDAs of solar-type stars. Abundances and PDAs are determined for 28 elements: C, N, O, Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Y, Zr, Ba, La, Ce, Nd, Sm, Eu, and Gd. A plot of PDAs ($\theta$ Scl minus Procyon) vs. $Z$ shows a highly significant correlation. Moreover, local substructure of the plot for the elements Ca-Zn and neutron-addition elements is similar to that which can be found for solar twins. Our PDA vs. $Z$ plot structural similarity to plots that can be made from the extensive work of Bedell et al. (2018). That PDA structure and substructure is clearly a function of age.

arXiv comment8 pages, 4 figures. Accepted for publication in Astronomische Nachrichten

References in corpus (25)

• The chemical composition of the Sun
• The peculiar solar composition and its possible relation to planet formation
• Spectral Properties of Cool Stars: Extended Abundance Analysis of 1617 Planet Search Stars
• The FIP and Inverse FIP Effects in Solar and Stellar Coronae
• The elemental composition of the Sun II. The iron group elements Sc to Ni
• High-precision abundances of elements in solar twin stars: Trends with stellar age and elemental condensation temperature
• ARES v2 - new features and improved performance
• Spectroscopic Signatures of Convection in the Spectrum of Procyon. Fundamental Parameters and Iron Abundance
• The elemental composition of the Sun III. The heavy elements Cu to Th
• The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood
• Improved Laboratory Transition Probabilities for Neutral Chromium and Re-determination of the Chromium Abundance for the Sun and Three Stars
• Improved Laboratory Transition Probabilities for Ce II, Application to the Cerium Abundances of the Sun and Five r-process Rich, Metal-Poor Stars, and Rare Earth Lab Data
• The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets
• Improved Ti II log(gf) Values and Abundance Determinations in the Photospheres of the Metal-Poor Star HD 84937
• Abundance to age ratios in the HARPS-GTO sample with Gaia DR2: Chemical clocks for a range of [Fe/H]
• The origin and evolution of the odd-Z iron-peak elements Sc, V, Mn, and Co in the Milky Way stellar disk
• Stellar Chemical Abundances: In Pursuit of the Highest Achievable Precision
• High-precision stellar abundances of the elements - methods and applications
• Chemical abundances of magnetic and non-magnetic Herbig Ae/Be stars
• Chemical signatures of planets: beyond solar-twins
• The abundance pattern of the lambda Bootis stars
• The Age and Stellar Parameters of the Procyon Binary System
• Non-LTE radiative transfer in cool stars. Theory and applications to the abundance analysis for 24 chemical elements
• The Belgian repository of fundamental atomic data and stellar spectra (BRASS) II. Quality assessment of atomic data for unblended lines in FGK stars
• Chemical abundances of the high-latitude Herbig Ae Star PDS2

Cited by in corpus (1)

• Investigating three Sirius-like systems with SPHERE