61 citations · 114 across the 5 of their papers we have counts for
5 papers
Three-dimensional hydrodynamical simulations of mass transfer in binary systems by a free wind
Zheng-Wei Liu, Richard J. Stancliffe, Carlo Abate +1
A large fraction of stars in binary systems are expected to undergo mass and angular momentum exchange at some point in their evolution, which can drastically alter the chemical an…
Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
E. Matrozis, R. J. Stancliffe
Carbon-enhanced metal-poor stars with s-process enrichment (CEMP-s) are believed to be the products of mass transfer from an AGB companion, which has long since become a white dwar…
How much mass and angular momentum can the progenitors of carbon-enriched stars accrete?
E. Matrozis, C. Abate, R. J. Stancliffe
The chemically peculiar barium stars, CH stars, and most CEMP stars are all believed to be the products of mass transfer in binary systems from a now extinct AGB primary star. The…
Radiative levitation in carbon-enhanced metal-poor stars with s-process enrichment
E. Matrozis, R. J. Stancliffe
A significant fraction of all metal-poor stars are carbon-rich. Most of these carbon-enhanced metal-poor (CEMP) stars also show enhancement in elements produced mainly by the s-pro…
On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
E. Matrozis, N. Ryde, A. K. Dupree
Context. The Galactic chemical evolution of sulphur is still under debate. At low metallicities some studies find no correlation between [S/Fe] and [Fe/H], others find [S/Fe] incre…