Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • THE EVOLUTION OF DISK GALAXIES: NATURE OR NURTURE? (LA EVOLUCIÓN DE GALAXIAS DE DISCO: ¿NATURALEZA O CREACIÓN?)
    VALERIA BUENROSTRO-LEITER

    Advertised on:

    11
    2009
  • THE EVOLUTION OF DISC GALAXIES:NATURE OR NURTURE? LA EVOLUCION DE GALAXIAS DE DISCO; ¿NATURALEZA O CREACION?
    Sabemos que hay varios procesos dinámicos en la Galaxia que pueden ser explicados con acreción de gas al disco Galáctico. Por ello hemos decidido investigar concretamente a las nubes de alta velocidad, o HVCs. Al estudiar al Complejo H, una nube en nuestra propia Galaxia que parece estar interaccionando con el disco Galáctico, encontramos que la
    Valeria Buenrostro Leiter

    Advertised on:

    11
    2009
  • The energy of waves in the photosphere and lower chromosphere. I. Velocity statistics
    Context: Acoustic waves are one of the primary suspects besides magnetic fields for the chromospheric heating process to temperatures above radiative equilibrium (RE). Aims: We derived the mechanical wave energy as seen in line-core velocities on disc centre to obtain a measure of mechanical energy flux with height for a comparison with the energy
    Beck, C. et al.

    Advertised on:

    11
    2009
    Citations
    38
  • The Chemical Composition of Cernis 52 (BD+31° 640)
    We present an abundance analysis of the star Cernis 52 in whose spectrum we recently reported the naphthalene cation in absorption at 6707.4 Å. This star is on a line of sight to the Perseus molecular complex. The analysis of high-resolution spectra using a χ2-minimization procedure and a grid of synthetic spectra provides the stellar parameters
    González Hernández, J. I. et al.

    Advertised on:

    11
    2009
    Citations
    14
  • The bright galaxy population of five medium redshift clusters. II. Quantitative galaxy morphology
    Aims: Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18 ≤ z ≤ 0.25 imaged in the central 0.5-2 Mpc in very good seeing conditions, we have studied the quantitative morphology of their bright galaxy population Methods: We
    Ascaso, B. et al.

    Advertised on:

    11
    2009
    Citations
    6