Updated stellar yields from asymptotic giant branch models
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 6 M⊙. New intermediate
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Karakas_Updated_stellar_yields_from_2010.pdf||1.2 MB||Adobe PDF||Request a copy|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.