S stars and s -process in the Gaia era - Université de Montpellier Accéder directement au contenu
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2021

S stars and s -process in the Gaia era

Shreeya Shetye
  • Fonction : Auteur
Sophie van Eck
  • Fonction : Auteur
Alain Jorissen
  • Fonction : Auteur
Stephane Goriely
  • Fonction : Auteur
Lionel Siess
  • Fonction : Auteur
Hans van Winckel
  • Fonction : Auteur
Michel Godefroid
  • Fonction : Auteur
George Wallerstein
  • Fonction : Auteur


Context. S stars are late-type giants that are transition objects between M-type stars and carbon stars on the asymptotic giant branch (AGB). They are classified into two types: intrinsic or extrinsic, based on the presence or absence of technetium (Tc). The Tc-rich or intrinsic S stars are thermally pulsing (TP-)AGB stars internally producing s -process elements (including Tc) that are brought to their surface via the third dredge-up (TDU). The Tc-poor or extrinsic S stars gained their s -process overabundances via the accretion of s -process-rich material from an AGB companion that has since turned into a dim white dwarf. Aims. Our goal is to investigate the evolutionary status of Tc-rich S stars by locating them in a Hertzsprung-Russell (HR) diagram using the results of Gaia Early Data Release 3 (EDR3). We combine the current sample of 13 Tc-rich stars with our previous studies of 10 Tc-rich stars to determine the observational onset of the TDU in the metallicity range [−0.7; 0]. We also compare our abundance determinations with dedicated AGB nucleosynthesis predictions. Methods. We derived the stellar parameters using an iterative tool that combines HERMES high-resolution spectra, accurate Gaia EDR3 parallaxes, stellar evolution models, and tailored MARCS model atmospheres for S-type stars. Using these stellar parameters, we determined the heavy-element abundances by line synthesis. Results. In the HR diagram, the intrinsic S stars are located at higher luminosities than the predicted onset of the TDU. These findings are consistent with Tc-rich S stars being genuine TP-AGB stars. The comparison of the derived s -process abundance profiles of our intrinsic S stars with the nucleosynthesis predictions provide an overall good agreement. Stars with highest [s/Fe] tend to have the highest C/O ratios.

Dates et versions

hal-03854997 , version 1 (16-11-2022)



Shreeya Shetye, Sophie van Eck, Alain Jorissen, Stephane Goriely, Lionel Siess, et al.. S stars and s -process in the Gaia era. Astronomy and Astrophysics - A&A, 2021, 650, pp.A118. ⟨10.1051/0004-6361/202040207⟩. ⟨hal-03854997⟩
15 Consultations
0 Téléchargements



Gmail Mastodon Facebook X LinkedIn More