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/

  • An UXor among FUors: Extinction-related Brightness Variations of the Young Eruptive Star V582 Aur
    V582 Aur is an FU Ori-type young eruptive star in outburst since ∼1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic variability superimposed. Here we will characterize the progenitor of the outbursting object, explore its environment, and analyze the temporal evolution of the eruption. We are
    Ábrahám, P. et al.

    Advertised on:

    1
    2018
    Citations
    26
  • An excess of massive stars in the local 30 Doradus starburst
    The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analog of large star-formation events in the distant universe. We determined the recent formation history and the initial mass function (IMF) of massive stars in 30 Doradus on the basis of spectroscopic observations of 247 stars more massive than 15 solar masses (M☉). The
    Schneider, F. R. N. et al.

    Advertised on:

    1
    2018
    Citations
    212
  • A HST/WFC3 Search for Substellar Companions in the Orion Nebula Cluster
    We present new results relative to the population of substellar binaries in the Orion Nebula Cluster. We reprocessed HST/WFC3 data using an analysis technique developed to detect close companions in the wings of the stellar PSFs, based on the PyKLIP implementation of the KLIP PSF subtraction algorithm. Starting from a sample of ~1200 stars selected
    Strampelli, G. M. et al.

    Advertised on:

    1
    2018
    Citations
    0
  • A dusty star-forming galaxy at z = 6 revealed by strong gravitational lensing
    Since their discovery, submillimetre-selected galaxies1,2 have revolutionized the field of galaxy formation and evolution. From the hundreds of square degrees mapped at submillimetre wavelengths3-5, only a handful of sources have been confirmed to lie at z > 5 (refs 6-10) and only two at z ≥ 6 (refs 11,12). All of these submillimetre galaxies are
    Zavala, J. A. et al.

    Advertised on:

    1
    2018
    Citations
    89
  • 280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope
    Context. One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to be too faint for detection in shallow surveys at future apparitions. Aims: We aimed to recover more than half of the one-opposition NEAs recommended for
    Vaduvescu, O. et al.

    Advertised on:

    1
    2018
    Citations
    13
  • Transit Photometry as an Exoplanet Discovery Method
    Photometry with the transit method has arguably been the most successful exoplanet discovery method to date. A short overview about the rise of that method to its present status is given. The method's strength is the rich set of parameters that can be obtained from transiting planets, in particular in combination with radial velocity observations
    Deeg, Hans J. et al.

    Advertised on:

    2018
    Citations
    20