Publication type: Refereed

  • Publication
    Galactic Interstellar Gas Cloud Mass Functions: A Simple Quantitative Approach
    We present here a simple approach to understanding the gas cloud mass distribution function by simulating formation and destruction of gas clouds and gas clumps...
  • Publication
    Galactic kinematics of Planetary Nebulae with [WC] central star
    High resolution spectra are used to analyze the galactic kinematics and distribution of a sample of planetary nebulae with [WR] and `wel' central star ([WR]PN...
  • Publication
    Galactic observatory science with the ASTRI Mini-Array at the Observatorio del Teide
    The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array will be composed of nine imaging atmospheric Cherenkov telescopes at the...
  • Publication
    Galactic planetary nebulae with precise nebular abundances as a tool to understand the evolution of asymptotic giant branch stars
    We present nucleosynthesis predictions (HeCNOCl) from asymptotic giant branch (AGB) models, with diffusive overshooting from all the convective borders, in the...
  • Publication
    Galactic planetary nebulae with Wolf-Rayet nuclei. I. Objects with [WC]-early type stars
    Spatially resolved long-slit spectrophotometric data for the planetary nebulae PB 6, NGC 2452, NGC 2867, NGC 6905 and He 2-55 are presented. Different knots...
  • Publication
    Galactic Populations of Radio and Gamma-Ray Pulsars in the Polar Cap Model
    We simulate the characteristics of the Galactic population of radio and γ-ray pulsars using Monte Carlo techniques. At birth, neutron stars are spatially...
  • Publication
    Galactic synchrotron emission at high frequencies
    The search for structure in the cosmic microwave background (CMB) needs to take into account the Galactic background contribution. The potential of using...
  • Publication
    Galactic warp in the overdensity of the Canis Major region
    Bellazzini et al. claim that López-Corredoira et al. warp model is totally unable to reproduce the Canis Major structure in the red clump stars. However, slight...
  • Publication
    Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
    The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven...