Publication type: Refereed

  • Publication
    An implicit integral method to solve selected radiative transfer problems. 2: LTE stellar atmosphere models
    The implicit intergral method that we have already introduced in a previous paper, together with its application to the non-Local Thermal Equilibrium (non-LTE)...
  • Publication
    An implicit integral method to solve selected radiative transfer problems. 3: Factorization versus linearization
    In view of more general applications, we have developed a new approach to render explicit the temperature both in the source function of the radiative transfer...
  • Publication
    An implicit integral method to solve selected radiative transfer problems. I - Non-LTE line formation
    In this paper we present a new method to solve those radiative transfer problems where the scattering term in the source function, i.e., the frequency...
  • Publication
    An Implicit Integral Method to Solve Selected Radiative Transfer Problems. IV. The Case of Spherical Geometry
    In the previous papers of this series, we introduced the implicit integral method (IIM) to solve those radiative transfer (RT) problems in which the source...
  • Publication
    An impressionist view of V Hydrae. When MATISSE paints asymmetric giant blobs
    Context. Asymptotic giant branch (AGB) stars enrich the interstellar medium through their mass loss. The mechanism(s) shaping the circumstellar environment of...
  • Publication
    An improved method for statistical studies of the internal kinematics of HII regions: the case of M83
    We present the integrated Hα emission line profile for 157 HII regions in the central 3.4 × 3.4 arcmin2 of the galaxy M83 (NGC 5236). Using the Fabry-Perot...
  • Publication
    An improved version of the implicit integral method to solving radiative transfer problems
    Radiative transfer (RT) problems in which the source function includes a scattering-like integral are typical two-points boundary problems. Their solution via...
  • Publication
    An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars
    Aims: The aim of this work was to use a multi-approach technique to derive the most accurate values possible of the physical parameters of the δ Sct star HD...
  • Publication
    An Infrared Census of DUST in Nearby Galaxies with Spitzer (DUSTiNGS). IV. Discovery of High-redshift AGB Analogs
    The survey for DUST in Nearby Galaxies with Spitzer (DUSTiNGS) identified several candidate Asymptotic Giant Branch (AGB) stars in nearby dwarf galaxies and...