Add to ORKGWe summarise the results of recent work investigating the effects of stellar yields which take into account rotation on the predictions of chemical evolution models for early populations of galaxies
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
We present a new set of stellar yields obtained from rotating stellar models at solar metallicity co...
[abridged] Many topical astrophysical research areas, such as the properties of planet host stars, t...
We compute the evolution of different abundance ratios in the Milky Way (MW) for two different sets ...
We compute the evolution of different abundance ratios in the Milky Way (MW) for two different sets ...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Context. Galactic chemical evolution models are useful tools for interpreting the large body of high...
We present a comparison between the [Ca,C,N/Fe]-mass relations observed in local spheroids and the r...
We calculate a grid of star models with and without the effects of axial rotation for stars in the m...
We review general characteristics of massive stars, present the main observable constraints that ste...
Context. Aims.We examine the role of rotation on the evolution and chemical yields of very metal-po...
We calculate a grid of star models with and without the effects of axial rotation for stars in the m...
For $^{12}$C and $^{16}$O, rotating models predict in general enhanced yields. At high metallicity, ...
We present a set of 144 Galactic chemical evolution models applied to a Milky Way analogue, computed...
We investigate the effect of new stellar models, which take rotation into account, computed for very...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
We present a new set of stellar yields obtained from rotating stellar models at solar metallicity co...
[abridged] Many topical astrophysical research areas, such as the properties of planet host stars, t...
We compute the evolution of different abundance ratios in the Milky Way (MW) for two different sets ...
We compute the evolution of different abundance ratios in the Milky Way (MW) for two different sets ...
Context. Although still beyond our observational abilities, Population III stars are interesting obj...
Context. Galactic chemical evolution models are useful tools for interpreting the large body of high...
We present a comparison between the [Ca,C,N/Fe]-mass relations observed in local spheroids and the r...
We calculate a grid of star models with and without the effects of axial rotation for stars in the m...
We review general characteristics of massive stars, present the main observable constraints that ste...
Context. Aims.We examine the role of rotation on the evolution and chemical yields of very metal-po...
We calculate a grid of star models with and without the effects of axial rotation for stars in the m...
For $^{12}$C and $^{16}$O, rotating models predict in general enhanced yields. At high metallicity, ...
We present a set of 144 Galactic chemical evolution models applied to a Milky Way analogue, computed...
We investigate the effect of new stellar models, which take rotation into account, computed for very...
Massive stars played a key role in the early evolution of the Universe. They formed with the first h...
We present a new set of stellar yields obtained from rotating stellar models at solar metallicity co...
[abridged] Many topical astrophysical research areas, such as the properties of planet host stars, t...