Research output per year
Research output per year
V. Pérez-Mesa, O. Zamora, D. A. García-Hernández, B. Plez, A. Manchado, A. I. Karakas, M. Lugaro
Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Other
We have explored the circumstellar effects on the Li abundance determination in a complete sample of O-rich Galactic asymptotic giant branch (AGB) stars, previously studied with hydrostatic models. We use a modified version of the spectral synthesis code Turbospectrum and more realistic extended model atmospheres that consider the presence of a gaseous circumstellar envelope and a radial wind in these massive AGB stars. The Li abundances are determined from the 6708 Å Li I resonance line. The Li pseudo-dynamical abundances obtained are practically identical to those derived with hydrostatic models (a maximum difference of 0.3 dex is found in the only super Li-rich AGB star in our sample). The low Li abundance and therefore negligible Li I column-density in the circumstellar envelope likely explains the small differences between extended and hydrostatic models. Our results confirm the activation of the hot bottom burning (HBB) process in massive Galactic AGB stars.
Original language | English |
---|---|
Title of host publication | Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society |
Subtitle of host publication | 2017 AGB-Supernovae Mass Transition; Monte Porzio Catone; Italy; 27 March 2017 through 31 March 2017 |
Editors | A Karakas, P Ventura, F Dell'Agli, M Di Criscienzo |
Place of Publication | Italy |
Pages | 451-454 |
Number of pages | 4 |
Volume | 88 |
Edition | 3 |
Publication status | Published - 2017 |
Event | The AGB-Supernovae Mass Transition 2017 - Observatory of Rome, Monte Porzio Catone, Italy Duration: 27 Mar 2017 → 31 Mar 2017 https://web.archive.org/web/20170111030144/http://agb-supernovae.weebly.com:80/ https://agb-supernovae.weebly.com/ |
Name | Memorie della Società Astronomica Italiana |
---|---|
Publisher | Società Astronomica Italiana |
ISSN (Print) | 0037-8720 |
Conference | The AGB-Supernovae Mass Transition 2017 |
---|---|
Country/Territory | Italy |
City | Monte Porzio Catone |
Period | 27/03/17 → 31/03/17 |
Other | Little is known about stars in the mass range between those that end their lives as white dwarfs and those that die in spectacular supernova explosions. The uncertainty stems from the fact that stars in this transition mass range from about ~7 to 11 solar masses are both difficult to model theoretically and there are few observational clues as to their evolutionary history. Following the ignition of carbon in the core under conditions of partial degeneracy, the stars then continue to evolve through the asymptotic giant branch (AGB) phase and are known as super-AGB stars. Super-AGB stars have oxygen-neon degenerate cores as opposed to the carbon-oxygen cores of their lower mass counterparts. The final fate of single super-AGB stars depends on the rate of mass loss from the surface: if the core can grow big enough to reach the Chandrasekhar mass then it will explode as an electron capture supernova. |
Internet address |
Research output: Contribution to journal › Article › Research › peer-review