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/

  • SPECTROSCOPIC PROPERTIES OF DWARF GALAXIES IN NEARBY CLUSTERS
    Desde el descubrimiento de que existen diferentes tipos de galaxias nos hemos preguntado sobre su formación y evolución. ¿Evolucionan de manera diferente las galaxias de distintos tamaños y masas? Las galaxias gigantes y masivas fueron las primeras en ser estudiadas, su alta luminosidad superficial permitió que los primeros telescopios las
    Jorge Romero Gómez

    Advertised on:

    9
    2024
  • X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars
    Context. The winds of massive stars have a significant impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows, the terminal wind speed v ∞, is a global wind parameter and an essential input for models of stellar atmospheres and feedback. With the arrival of the ULLYSES programme, a legacy UV
    Hawcroft, C. et al.

    Advertised on:

    8
    2024
    Citations
    31
  • X-Shooting ULLYSES: Massive stars at low metallicity. II. DR1: Advanced optical data products for the Magellanic Clouds
    Context. The XShootU project aims to obtain ground-based optical to near-infrared spectroscopy of all targets observed by the Hubble Space Telescope (HST) under the Director's Discretionary program ULLYSES. Using the medium-resolution spectrograph X-shooter, spectra of 235 OB and Wolf-Rayet (WR) stars in subsolar metallicity environments have been
    Sana, H. et al.

    Advertised on:

    8
    2024
    Citations
    10
  • Wind tunnel test for the preliminary design of the European Solar Telescope
    The European Solar Telescope (EST) is a 4.2-m solar telescope, based on an aplanatic Gregorian configuration with an alt-azimuthal mount. EST has an open configuration for observations without dome to improve the local seeing around the telescope mount and the main optical elements, enhancing the natural air flushing through the structure. This
    Urrutia, Ander et al.

    Advertised on:

    8
    2024
    Citations
    0
  • Using gas kinematics to measure resonant structures in disc galaxies: the interaction of M51 with NGC 5195
    Interstellar gas offers advantages when quantifying the structure of the resonances in disc galaxies. The gas is concentrated close to the disc mid-plane, making it easier to determine its in-plane velocity components, and it offers sharp emission lines for good velocity resolution. These properties are shared by atomic, molecular, and ionized gas
    Font, Joan et al.

    Advertised on:

    8
    2024
    Citations
    0
  • Upgrading the polarisation modulation unit of the Gregor Infrared Spectrograph
    The Gregor Infrared Spectrograph (GRIS) is installed at the Gregor telescope at Observatorio del Teide, Spain. The instrument started observations in 2012 and underwent several upgrades in the following years. Currently, it is experiencing the most significant upgrade so far, which includes, among other things, adding two optical channels to
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Citations
    0