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
    X-Ray Variability in LINERs
    Active galactic nuclei (AGN) are powered by energetic phenomena which cannot be attributed to stars. LINERs appears to be the low power end of the AGN sequence with the lowest Eddington ratios but hosting the most massive black holes (typically 109 M&sun;). Whereas variability is common for high Eddington ratio emitting sources, in the low
    Márquez, I. et al.

    Advertised on:

    2
    2013
    Bibcode
    2013IAUS..290...41H
    Citations
    0
  • Refereed
    Volatile and refractory abundances of F- and G-type stars
    We present a detailed chemical abundance analysis of a sample of F- and G-type stars. We investigate the possibility that the presence of terrestrial planets could affect the volatile-to-refractory abundance ratios. Stars with and without planets exhibit very similar abundance behaviours, either for solar twins or even when considering the whole
    Udry, S. et al.

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    2
    2013
    Bibcode
    2013AN....334..172G
    Citations
    3
  • Refereed
    Virgo cluster and field dwarf ellipticals in 3D - I. On the variety of stellar kinematic and line-strength properties
    We present the first large-scale stellar kinematic and line-strength maps for dwarf elliptical galaxies (nine in the Virgo cluster and three in the field environment) obtained with the SAURON (Spectrographic Areal Unit for Research on Optical Nebulae) integral-field unit. No two galaxies in our sample are alike: we see that the level of rotation is
    van de Ven, Glenn et al.

    Advertised on:

    2
    2013
    Bibcode
    2013MNRAS.428.2980R
    Citations
    53
  • Refereed
    The VLT-FLAMES Tarantula Survey. X. Evidence for a bimodal distribution of rotational velocities for the single early B-type stars
    Aims: Projected rotational velocities (vesini) have been estimated for 334 targets in the VLT-FLAMES Tarantula Survey that do not manifest significant radial velocity variations and are not supergiants. They have spectral types from approximately O9.5 to B3. The estimates have been analysed to infer the underlying rotational velocity distribution
    Dufton, P. L. et al.

    Advertised on:

    2
    2013
    Bibcode
    2013A&A...550A.109D
    Citations
    138
  • Refereed
    The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population
    Context. The Tarantula Nebula in the Large Magellanic Cloud is our closest view of a starburst region and is the ideal environment to investigate important questions regarding the formation, evolution and final fate of the most massive stars. Aims: We analyze the multiplicity properties of the massive O-type star population observed through multi
    Sana, H. et al.

    Advertised on:

    2
    2013
    Bibcode
    2013A&A...550A.107S
    Citations
    505
  • Refereed
    The VLT-FLAMES Tarantula Survey. IX. The interstellar medium seen through diffuse interstellar bands and neutral sodium&
    Context. The Tarantula Nebula (a.k.a. 30 Dor) is a spectacular star-forming region in the Large Magellanic Cloud (LMC), seen through gas in the Galactic disc and halo. Diffuse interstellar bands (DIBs) offer a unique probe of the diffuse, cool-warm gas in these regions. Aims: The aim is to use DIBs as diagnostics of the local interstellar
    van Loon, J. Th. et al.

    Advertised on:

    2
    2013
    Bibcode
    2013A&A...550A.108V
    Citations
    72