The impact of axion-like particles on late stellar evolution - From intermediate-mass stars to core-collapse supernova progenitors

Open Access

Fig. 8.

Contours of Δ $M_{COWD}^{\max}$ $M^{\mathrm{max}}_{\mathrm{COWD}}$ , in steps of 0.2 M_⊙ in the g_ae - g_aγ plane, considering the current bounds. The projected sensitivity of Baby IAXO and IAXO are also indicated for reference, as this is the area excluded by the CAST result.

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.