Open Access

Fig. 1.

image

Download original image

Carbon-oxygen core mass (MCO) versus the central 12C mass fraction abundance (XC12) at the end of central He burning phase. The different colors identify the different sets of models (see side legend) where RAU is Rauscher et al. (2002); PGN is Pignatari et al. (2016); SIE is Sieverding et al. (2018); RIT is Ritter et al. (2018a); L&C is Limongi & Chieffi (2018); BRI is Brinkman et al. (2019, 2021); LIM is Limongi et al. (2024); RLC is Roberti et al. (2024a); ROB is Roberti et al. (2024b); and KEP is Jeena et al. (2024). Different symbols identify different initial masses (see top legend). Models with and without a C-O shell merger are represented by filled and empty symbols, respectively. The two gray shaded areas represent the covariant confidence ellipses relative to the models with C-O mergers within one and two standard deviations, σ, centred at MCO = 4.02 and XC12 = 0.176.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.