Publication type: Refereed

  • Publication
    Evolutionary synthesis models for the emission from radioactive isotopes in H II regions
    We have extended our evolutionary synthesis models for Star Forming Regions to the γ-ray domain. Applying different yields to the resulting synthetic...
  • Publication
    Evolutionary synthesis models of starbursts. IV. Soft X-ray emission
    In this work we investigate the evolution of the X-ray emission of a cluster of single young massive stars with different metallicities. We have considered the...
  • Publication
    Evolutionary Synthesis Models: Gamma-ray Emission
    Not Available
  • Publication
    Evolutionary versus dynamical time scales for the evolution of the central stars of planetary nebulae
    The disagreement between evolutionary and dynamical time scales for the evolution of the central stars of planetary nebulae (CSPN) through the H-R diagram is...
  • Publication
    Evolved stars in the Local Group galaxies - I. AGB evolution and dust production in IC 1613
    We used models of thermally pulsing asymptotic giant branch (AGB) stars, which also describe the dust-formation process in the wind, to interpret the...
  • Publication
    Evolved stars in the Local Group galaxies - II. AGB, RSG stars, and dust production in IC10
    We study the evolved stellar population of the Local Group galaxy IC10, with the aim of characterizing the individual sources observed and to derive global...
  • Publication
    Evolved stars in the Local Group galaxies - III. AGB and RSG stars in Sextans A
    We study the evolved stellar population of the galaxy Sextans A. This galaxy is one of the lowest metallicity dwarfs in which variable asymptotic giant branch...
  • Publication
    Evolved stars suggest an external origin of the enhanced metallicity in planet-hosting stars
    Aims: Exo-planets are preferentially found around high metallicity main sequence stars. We investigate whether evolved stars share this property, and its...
  • Publication
    EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey
    Context. With a mass exceeding several 10 4 M ⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive...