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Showing 2020 · astro-ph.SRShow all
3 papers · 2 filters
astro-ph.SR2020★ 9 cited
Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clusters
S. Martocchia, S. Kamann, S. Saracino +13
Ancient (10 Gyr) globular clusters (GCs) show chemical abundance variations in the form of patterns among certain elements, e.g. N correlates with Na and anti-correlates with O.…
astro-ph.SR2020★ 56 cited
The interpretation of protoplanetary disc wind diagnostic lines from X-ray photoevaporation and analytical MHD models
Michael L. Weber, Barbara Ercolano, Giovanni Picogna +2
High resolution spectra of typical wind diagnostics ([OI] 6300 Å and other forbidden emission lines) can often be decomposed into multiple components: high-velocity components with…
astro-ph.SR2020★ 20 cited
Impact of Convective Boundary Mixing on the TP-AGB
Graham Wagstaff, Marcelo M. Miller Bertolami, Achim Weiß
The treatment of convective boundaries remains an important source of uncertainty within stellar evolution, with drastic implications for the thermally-pulsing stars on the Asympto…