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/

  • Indication of the Hanle Effect by Comparing the Scattering Polarization Observed by CLASP in the Lyα and Si iii 120.65 nm Lines
    The Chromospheric Lyman-Alpha Spectro-Polarimeter is a sounding rocket experiment that has provided the first successful measurement of the linear polarization produced by scattering processes in the hydrogen Lyα line (121.57 nm) radiation of the solar disk. In this paper, we report that the Si iii line at 120.65 nm also shows scattering
    Ishikawa, R. et al.

    Advertised on:

    5
    2017
    Citations
    16
  • Identification of Near-infrared [Se iii] and [Kr vi] Emission Lines in Planetary Nebulae
    We identify [Se iii] 1.0994 μm in the planetary nebula (PN) NGC 5315 and [Kr vi] 1.2330 μm in three PNe from spectra obtained with the Folded-Port InfraRed Echellette (FIRE) spectrometer on the 6.5 m Baade Telescope. Se and Kr are the two most widely detected neutron-capture elements in astrophysical nebulae, and can be enriched by s-process
    Sterling, N. C. et al.

    Advertised on:

    5
    2017
    Citations
    17
  • Hints on the Gradual Resizing of the Torus in AGNs through Decomposition of Spitzer/IRS Spectra
    Several authors have claimed that less luminous active galactic nuclei (AGNs) are not capable of sustaining a dusty torus structure. Thus, a gradual resizing of the torus is expected when the AGN luminosity decreases. Our aim is to examine mid-infrared observations of local AGNs of different luminosities for the gradual resizing and disappearance
    González-Martín, Omaira et al.

    Advertised on:

    5
    2017
    Citations
    28
  • Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects
    Context. The first Gaia Data Release contains the Tycho-Gaia Astrometric Solution (TGAS). This is a subset of about 2 million stars for which, besides the position and photometry, the proper motion and parallax are calculated using Hipparcos and Tycho-2 positions in 1991.25 as prior information. Aims: We investigate the scientific potential and
    Zschocke, S. et al.

    Advertised on:

    5
    2017
    Citations
    94
  • Evidence of chaotic modes in the analysis of four δ Scuti stars
    Context. Since CoRoT observations unveiled the very low amplitude modes that form a flat plateau in the power spectrum structure of δ Scuti stars, the nature of this phenomenon, including the possibility of spurious signals due to the light curve analysis, has been a matter of long-standing scientific debate. Aims: We contribute to this debate by
    Barceló-Forteza, S. et al.

    Advertised on:

    5
    2017
    Citations
    17
  • CHEMICAL ABUNDANCES OF VOLATILE AND REFRACTORY ELEMENTS IN STARS WITH AND WITHOUT EXOPLANETS
    Since the 1995 discovery of the first exoplanet orbiting a solar-type star (Mayor & Queloz 1995), the number of these has grown exponentially. To date, more than 4,500 planets have been detected (more than 3,200 confirmed). In addition, the size of these planets is very diverse, from giant Jupiter-type planets (the first to be discovered) to Earth
    Lucía Suárez Andrés

    Advertised on:

    5
    2017