327 citations · 3.7k across the 84 of their papers we have counts for
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Light element abundances in carbon-enhanced metal-poor stars
Richard J. Stancliffe
We model the evolution of the abundances of light elements in carbon-enhanced metal-poor (CEMP) stars, under the assumption that such stars are formed by mass transfer in a binary…
Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars
Richard J. Stancliffe, Evert Glebbeek
We investigate the formation of carbon-enhanced metal-poor (CEMP) stars via the scenario of mass transfer from a carbon-rich asymptotic giant branch (AGB) primary to a low-mass com…
An Explosive End to Intermediate-Mass Zero-Metallicity Stars and Early Universe Nucleosynthesis
H. B. Lau, R. J. Stancliffe, C. A. Tout
We use the Cambridge stellar evolution code STARS to model the evolution of 5-7 solar mass zero-metallicity stars. With enhanced resolution at the hydrogen and helium burning shell…
Impact of Rotation on the Evolution of Low-Mass Stars
D. Brown, M. Salaris, S. Cassisi +1
High precision photometry and spectroscopy of low-mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar…
The Impact of Rotation on the Evolution of Low-Mass Stars
D. Brown, M. Salaris
High precision photometry and spectroscopy of low-mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar…
The effect of different opacity data and chemical element mixture on the Petersen diagram
P. Lenz, A. A. Pamyatnykh, M. Breger
The Petersen diagram is a frequently used tool to constrain model parameters such as metallicity of radial double-mode pulsators. In this diagram the period ratio of the radial fir…