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/

  • Non-refereed
    Ultraviolet emission line imaging of planetary nebulae with GALEX
    GALEX (the Galaxy Evolution Explorer) has provided far-UV(1344-1786Å) and near-UV(1771-2831Å) imaging of several Planetary Nebulae (e.g., Bianchi et al. 2008, Bianchi 2012), with flux limits ~27.5 mag/sq.arcsec for objects in the Medium-deph Imaging Survey (MIS). PNe images in the GALEX broad-band UV filters include flux from both nebular line and
    Bianchi, Luciana et al.

    Advertised on:

    8
    2012
    Bibcode
    2012IAUS..283..308B
    Citations
    5
  • Non-refereed
    Unravelling the role of SW Sextantis stars in the evolution of cataclysmic variables
    SW Sextantis stars are a relatively large group of cataclysmic variables whose properties contradict all predictions made by the current CV evolution theories. Very little is known about the properties of their accreting white dwarfs and their donor stars, as the stellar components are usually outshone by an extremely bright accretion flow
    Araujo-Betancor, Sofia et al.

    Advertised on:

    8
    2005
    Bibcode
    2005noao.prop...23A
    Citations
    0
  • Non-refereed
    Unravelling the Role of the SW Sextantis Stars in the Evolution of Cataclysmic Variables
    SW Sextantis stars are a relatively large group of cataclysmic variables whose properties contradict all predictions made by the current CV evolution theories. Very little is known about the properties of their accreting white dwarfs and their donor stars, as the stellar components are usually outshone by an extremely bright accretion flow
    Torres, Manuel et al.

    Advertised on:

    8
    2006
    Bibcode
    2006noao.prop..566T
    Citations
    0
  • Non-refereed
    Unravelling the role of the SW Sextantis stars in the evolution of cataclysmic variables
    SW Sextantis stars are a relatively large group of cataclysmic variables (CVs) whose properties contradict all predictions made by the current CV evolution theories. Very little is known about the properties of their accreting white dwarfs and their donor stars, as the stellar components are usually outshone by an extremely bright accretion flow
    Torres, Manuel et al.

    Advertised on:

    8
    2007
    Bibcode
    2007noao.prop...51T
    Citations
    0
  • Refereed
    Unusual high-frequency oscillations in the Kepler δ Scuti star KIC 4840675
    We show that the star KIC 4840675 observed by Kepler is composed of three stars with a rapidly rotating A-type star and two solar-type fainter companions. The A-type star is a δ Scuti variable with a dominant mode and many other modes of lower amplitude, including several low-frequency variations. The low-frequency variation with highest amplitude
    Balona, L. A. et al.

    Advertised on:

    8
    2012
    Bibcode
    2012MNRAS.424.1187B
    Citations
    11
  • Non-refereed
    Upholding the unified model for AGN: VLT/FORS2 spectropolarimetry of Seyfert 2 galaxies
    The origin of the unification model for AGN was the detection of broad hydrogen recombination lines in the optical polarized spectrum of the Seyfert 2 galaxy (Sy2) NGC 1068. Since then, a search for the hidden broad-line region (HBLR) of nearby Sy2s started, but polarized broad lines have only been detected in ~30-40% of the nearby Sy2s observed to
    Ramos Almeida, C. et al.

    Advertised on:

    8
    2016
    Bibcode
    2016agnw.confE..52R
    Citations
    0