Updated stellar yields from AGB models (Karakas, 2010)

Details Updated stellar yields from AGB models (Karakas, 2010) Updated stellar yields from AGB models (Karakas, 2010)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..74031413k&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/403/1413. Originally published in: 2010MNRAS.403.1413K

Computer Science

Models, Stars: Giant, Abundances

Scientific paper

An updated grid of stellar yields for low- to intermediate-mass thermally pulsing asymptotic giant branch (AGB) stars is presented. The models cover a range in metallicity Z=0.02, 0.008, 0.004 and 0.0001, and masses between 1 and 6M&sun;. New intermediate-mass (M>=3M&sun;) Z=0.0001 AGB models are also presented, along with a finer mass grid than used in previous studies. The yields are computed using an updated reaction rate network that includes the latest NeNa and MgAl proton capture rates.
(6 data files).

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