Tipo de publicación: Sin árbitro

  • Publicación
    Enanas blancas post-AGB deficientes en Hidrógeno: su evolución espectral PG1159-DB-DQ
    This work explore the formation and evolution of hydrogen-deficient post-AGB white dwarfs. To this end, we compute the complete evolution of an initially 2.7 M...
  • Publicación
    End-to-end simulation framework for astronomical spectrographs: SOXS, CUBES, and ANDES
    We present our numerical simulation approach for the End-to-End (E2E) model applied to various astronomical spectrographs, such as SOXS (ESO-NTT), CUBES (ESO...
  • Publicación
    Energy implications of temperature fluctuations
    We quantify the energy radiated through all the collisional lines in a photoionized nebula in the presence of temperature fluctuations in the form of hot spots...
  • Publicación
    Enhancements over the electronic control for OSIRIS-Gtc Fabry-Perot tunable filters.
    OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the optical Day One instrument for the 10.4m Spanish telescope GTC (Gran...
  • Publicación
    Enhancing WFIRST Science with the Addition of a Redder Filter
    We outline a number of science advantages for adding a K or Ks filter (lambda_c 2.15 microns) and propose to extend the wavelength coverage for WFIRST into the...
  • Publicación
    Enigmatic Low-Velocity Jet-Like Features in Planetary Nebulae
    We are developing a project aimed at studying the physical properties, origin and evolution of low-ionization structures in planetary nebulae. Within this...
  • Publicación
    Entrega de IMaX al globo polar SUNRISE
    Not Available
  • Publicación
    Environmental dependence of the IMF-sensitive features in intermediate-mass quiescent galaxies
    In this work, we investigate the impact of large-scale environment on the IMF in quiescent galaxies. For this purpose, we compare the trend of IMF-sensitive...
  • Publicación
    Environmental effects in the structural parameters of Coma galaxies
    We have studied the quantitative morphology of the galaxies of the Coma cluster brighter than mr=17. The surface brightness profiles of all galaxies were...