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
    Spectrophotometric study in the near-IR of a sample of H alpha-selected galaxies with active star formation at z = 0.84
    In this work we present the results of the spectroscopic analysis in the near-infrared J band of a sample of 48 star forming galaxies at z = 0.84. Half of the sample was selected by a narrow-band filter tuned to Hα at that redshift and the other half was selected by photometric redshifts at the same redshift. We provide Hα luminosities and star
    Sánchez de Miguel, A. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011hsa6.conf..328S
    Citations
    0
  • Non-refereed
    Size evolution of massive galaxies
    We present the preliminary results of cosmological simulation focused on the study of the size and velocity dispersion time evolution. We have study the main morphological features of a sample of more that 200 galaxies having masses between 5 x 10^{10} M_&sun; and 5 x 10^{11} M_&sun;. We compared the results obtained from the analysis of the
    Navarro-González, J. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011hsa6.conf..393N
    Citations
    0
  • Refereed
    Shock-induced polarized hydrogen emission lines in the Mira star o Ceti
    Context. In the spectra of variable pulsating stars, especially Mira stars, the detection of intense hydrogen emission lines has been explained by the presence of a radiative and hypersonic shock wave, periodically propagating throughout the stellar atmosphere. Previous observation of the Mira star o Ceti around one of its brightest maximum light
    Fabas, N. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011A&A...535A..12F
    Citations
    15
  • Non-refereed
    Shaping massive galaxies: their morphology and kinematics at z = 1-3
    Massive (M_* ≥ 10^{11} M_&sun;) galaxies at high redshift (z ≥ 1.5) remain mysterious objects. Their extremely small sizes (effective radii of 1-2 kpc) make them as dense as modern globular clusters. It is thought that a highly dissipational merger is needed to create such compact galaxies. Within this proceedings, we discuss this issue, along with
    Buitrago, F. et al.

    Advertised on:

    11
    2011
    Bibcode
    2011hsa6.conf..154B
    Citations
    0