The intermediate-age Magellanic Cloud clusters NGC 1978 and 419 are each found to contain substantial numbers of pulsating asymptotic giant branch (AGB) stars, both oxygen rich and carbon rich. Each cluster also contains two pulsating AGB stars which ar
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...
This article compares the distribution of Ks magnitudes of Large Magellanic Cloud (LMC) asymptotic g...
The intermediate-age Magellanic Cloud clusters NGC 1978 and 419 are each found to contain substantia...
In this work we study the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) stars in the Small Mag...
The presence of asymptotic giant branch (AGB) stars in clusters provides key constraints for stellar...
Aims.We investigate variability and we model the pulsational behaviour of AGB variables in the inter...
We present the latest results of a theoretical project aimed at investigating the properties of ther...
High-dispersion near-infrared spectra have been taken of seven highly evolved, variable, intermediat...
Benefiting from the Gala second and early third releases of photometric and astrometric data, we exa...
To construct a catalogue of oxygen-rich (M) asymptotic giant branch (AGB) stars in the halo, complem...
10 pages, 12 figs, 3 Tables. Accepted for publication by AAInternational audienceTo construct a cata...
Multiple stellar populations (MPs) are a common feature of Globular Clusters (GCs). Their general pr...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
Multiple stellar populations (MPs) are a distinct characteristic of globular clusters (GCs). Their g...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...
This article compares the distribution of Ks magnitudes of Large Magellanic Cloud (LMC) asymptotic g...
The intermediate-age Magellanic Cloud clusters NGC 1978 and 419 are each found to contain substantia...
In this work we study the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) stars in the Small Mag...
The presence of asymptotic giant branch (AGB) stars in clusters provides key constraints for stellar...
Aims.We investigate variability and we model the pulsational behaviour of AGB variables in the inter...
We present the latest results of a theoretical project aimed at investigating the properties of ther...
High-dispersion near-infrared spectra have been taken of seven highly evolved, variable, intermediat...
Benefiting from the Gala second and early third releases of photometric and astrometric data, we exa...
To construct a catalogue of oxygen-rich (M) asymptotic giant branch (AGB) stars in the halo, complem...
10 pages, 12 figs, 3 Tables. Accepted for publication by AAInternational audienceTo construct a cata...
Multiple stellar populations (MPs) are a common feature of Globular Clusters (GCs). Their general pr...
In the recent controversy about the role of thermally pulsing asymptotic giant branch (TP-AGB) stars...
Multiple stellar populations (MPs) are a distinct characteristic of globular clusters (GCs). Their g...
In spite of its relevance, the Thermally Pulsing Asymptotic Giant Branch (TP-AGB) phase is one of th...
Asymptotic giant branch (AGB) stars are simultaneously one of the most important and least well unde...
This article compares the distribution of Ks magnitudes of Large Magellanic Cloud (LMC) asymptotic g...