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/

  • A lower limit to the accretion disc radius in the low-luminosity AGNNGC 1052 derived from high-angular resolution data
    We investigate the central sub-arcsec region of the low-luminosity active galactic nucleusNGC 1052, using a high-angular resolution data set that covers 10 orders of magnitude in frequency. This allows us to infer the continuum emission within the innermost ˜17 pc around the black hole to be of non-thermal, synchrotron origin and to set a limit to
    Reb, L. et al.

    Advertised on:

    7
    2018
    Citations
    10
  • A 15.7-minAM CVn binary discovered in K2
    We present the discovery of SDSS J135154.46-064309.0, a short-period variable observed using 30-mincadence photometry in K2 Campaign 6. Follow-up spectroscopy and high-speed photometry support a classification as a new member of the rare class of ultracompact accreting binaries known as AM CVn stars. The spectroscopic orbital period of 15.65 ± 0.12
    Green, M. J. et al.

    Advertised on:

    7
    2018
    Citations
    24
  • 3D Asymmetrical motions of the Galactic outer disc with LAMOST K giant stars
    We present a three dimensional velocity analysis of Milky Way disc kinematics using LAMOST K giant stars and the GPS1 proper motion catalogue. We find that Galactic disc stars near the anticentre direction (in the range of Galactocentric distance between R = 8 and 13 kpc and vertical position between Z = -2 and 2 kpc) exhibit asymmetrical motions
    Wang, H. et al.

    Advertised on:

    7
    2018
    Citations
    43
  • ERUPTIVE PHENOMENA IN THE SOLAR ATMOSPHERE: RADIATION-MHD MODELING AND CODE DEVELOPMENT
    A bewildering variety of eruptive and ejective phenomena continually take place in the solar atmosphere on a wide range of space and time scales. Particular attention was devoted in the past decades to those associated with the reconnection of magnetic field lines of separate plasma systems that come into contact in the atmosphere, especially when
    Daniel Nóbrega Siverio

    Advertised on:

    7
    2018
  • WINERED as a Stepping Stone for the Cosmic Distance Scale
    We present the Oscillating Stars with wIneRed near-Infrared Spectroscopy (OSIRIS) project, aimed at deriving accurate chemical abundances of primary distance indicators covering a wide age range from young Classical Cepheids to intermediate-age Anomalous Cepheids and Miras, old RR Lyrae stars, and Type-II Cepheids. High-resolution near-infrared
    Monelli, Matteo et al.

    Advertised on:

    6
    2018
    Citations
    0
  • The Transiting Exoplanet Community Early Release Science Program for JWST
    The James Webb Space Telescope offers astronomers the opportunity to observe the composition, structure, and dynamics of transiting exoplanet atmospheres with unprecedented detail. However, such observations require very precise time-series spectroscopic monitoring of bright stars and present unique technical challenges. The Transiting Exoplanet
    Berta-Thompson, Zachory K. et al.

    Advertised on:

    6
    2018
    Citations
    0