VizieR Online Data Catalog: Yields for Z=1e-5 intermediate-mass stars (Gil-Pons+, 2021)
Abstract
We tabulate nucleosynthetic yields and additional related information for intermediate-mass stars of metallicity Z=0.00001. These yields are the result of postprocessing of structure evolution obtained with MONSTAR (Monash and Mount Stromlo stellar evolution code). See Frost & Lattanzio, 1996ApJ...473..383F, Campbell & Lattanzio, 2008A&A...490..769C, Cat. J/A+A/490/769, and Gil-Pons et al. (2018PASA...35...38G). Interior stellar opacities are from Iglesias & Rogers (1996ApJ...464..943I). Variable-composition low-temperature opacity tables are from Lederer & Aringer (2009A&A...494..403L, Cat. J/A+A/494/403) and Marigo & Aringer (2009A&A...508.1539M). Initial composition was solar scaled as in Grevesse & Noels (1993PhST...47..133G). Stellar wind prescriptions are from Bloecker, 1995A&A...297..727B (Blo95) and from Vassiliadis and Wood, 1993ApJ...413..641V (VW93).
Postprocessing was calculated with the code MONSOON developed at Monash University (Cannon, 1993MNRAS,253,,817C; Lugaro et al., 2004ApJ...615..934L; Doherty et al., 2014MNRAS.437..195D). Nuclear reaction rates are mostly from the JINA reaction library (Cyburt et al., 2010ApJS..189..240C). p-captures for the NeNa-cycle and MgAl chain are from Iliadis et al. (2001ApJS..134..151I), p-captures on 22Ne are from Hale et al. (2002PhRvC..65a5801H, alpha-captures on 22Ne are from Karakas et al. (2006ApJ...643..471K), and p-captures on 23Na are from Hale et al. (2004PhRvC..70d5802H. The version of MONSOON used for the present work includes 77 species, up to 32S and Fe-peak elements. Additionally, it includes a 'g' particle (Lugaro et al., 2004ApJ...615..934L), which is a proxy for s-process elements. (2 data files).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- November 2020
- DOI:
- 10.26093/cds/vizier.36450010
- Bibcode:
- 2020yCat..36450010G
- Keywords:
-
- Models: evolutionary;
- Stars: carbon;
- Stars: metal-deficient;
- Stars: population II;
- Abundances