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/

  • Tracing Helioseismic Waves from the Photosphere to the Corona
    Can p-mode waves in sunspots propagate to the chromosphere and the corona? And what are their counterparts in different atmospheric heights? In order to study the connection between the photospheric p-mode waves and the waves observed above the photosphere, we use a helioseismic analysis technique, namely time-distance helioseismology, and analyze
    Zhao, J. et al.

    Advertised on:

    5
    2016
    Citations
    0
  • The Veritas and Themis asteroid families: 5-14 μm spectra with the Spitzer Space Telescope
    Spectroscopic investigations of primitive asteroid families constrain family evolution and composition and conditions in the solar nebula, and reveal information about past and present distributions of volatiles in the solar system. Visible and near-infrared studies of primitive asteroid families have shown spectral diversity between and within
    Landsman, Z. A. et al.

    Advertised on:

    5
    2016
    Citations
    14
  • The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II λ1640 in young star clusters
    We introduce a Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph (STIS) stellar census of R136a, the central ionizing star cluster of 30 Doradus. We present low resolution far-ultraviolet STIS spectroscopy of R136 using 17 contiguous 52 arcsec × 0.2 arcsec slits which together provide complete coverage of the central 0.85 parsec (3
    Crowther, P. A. et al.

    Advertised on:

    5
    2016
    Citations
    215
  • The possible origin of facular brightness in the solar atmosphere
    This paper studies the dependence of the Ca ii H line core brightness on the strength and inclination of the photospheric magnetic field, and on the parameters of convective and wave motions in a facular region at the center of the solar disc. We use three simultaneous data sets that were obtained at the German Vacuum Tower Telescope (Observatorio
    Kostik, R. et al.

    Advertised on:

    5
    2016
    Citations
    17
  • The OCCASO survey: presentation and radial velocities of 12 Milky Way open clusters
    Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. However, the lack of a large number of OCs analysed homogeneously hampers the investigations about chemical patterns and the existence of Galactocentric radial and vertical gradients, or an age-metallicity relation. To overcome this, we have designed the
    Casamiquela, L. et al.

    Advertised on:

    5
    2016
    Citations
    45
  • The Low Redshift survey at Calar Alto (LoRCA)
    The Baryon Acoustic Oscillation (BAO) feature in the power spectrum of galaxies provides a standard ruler to measure the accelerated expansion of the Universe. To extract all available information about dark energy, it is necessary to measure a standard ruler in the local, z 0.2, universe where dark energy dominates most the energy density of the
    Comparat, J. et al.

    Advertised on:

    5
    2016
    Citations
    6