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
    The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Overview and Membership Methods
    The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set for hundreds of open clusters, and constrain key Galactic dynamical and chemical parameters using the SDSS/APOGEE survey. We present the sample and methods being used by the survey to determine membership for the few-star
    Donor, J. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017AAS...22934301D
    Citations
    0
  • Non-refereed
    The Open Cluster Chemical Abundances and Mapping (OCCAM) Survey: Galactic Gradients using SDSS-IV/DR13 and Gaia
    The Open Cluster Chemical Analysis and Mapping (OCCAM) survey aims to produce a comprehensive, uniform, infrared-based data set forhundreds of open clusters, and constrain key Galactic dynamical and chemical parameters using the SDSS/APOGEE survey. We report on multi-element radial abundance gradients obtained from a sample of over 30 disk open
    Frinchaboy, P. M. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017AAS...22934302F
    Citations
    0
  • Refereed
    The inner mass distribution of late-type spiral galaxies from <monospace>SAURON</monospace> stellar kinematic maps
    We infer the central mass distributions within 0.4-1.2 disc scalelengths of 18 late-type spiral galaxies using two different dynamical modelling approaches - the asymmetric drift correction (ADC) and axisymmetric Jeans anisotropic multi-Gaussian expansion (JAM) model. ADC adopts a thin-disc assumption, whereas JAM does a full line-of-sight velocity
    Kalinova, V. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017MNRAS.464.1903K
    Citations
    19
  • Refereed
    The IACOB project. IV. New predictions for high-degree non-radial mode instability domains in massive stars and their connection with macroturbulent broadening
    Context. Asteroseismology is a powerful tool to access the internal structure of stars. Apart from the important impact of theoretical developments, progress in this field has been commonly associated with the analysis of time-resolved observations. Recently, the so-called macroturbulent broadening has been proposed as a complementary and less
    Godart, M. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017A&A...597A..23G
    Citations
    28
  • Refereed
    The IACOB project . III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars
    Context. The term macroturbulent broadening is commonly used to refer to a certain type of non-rotational broadening affecting the spectral line profiles of O- and B-type stars. It has been proposed to be a spectroscopic signature of the presence of stellar oscillations; however, we still lack a definitive confirmation of this hypothesis. Aims: We
    Simón-Díaz, S. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017A&A...597A..22S
    Citations
    149
  • Refereed
    The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. VIII. Preliminary Public Catalog Release
    The Hubble Space Telescope (HST) UV Legacy Survey of Galactic Globular Clusters (GO-13297) has been specifically designed to complement the existing F606W and F814W observations of the Advanced Camera for Surveys (ACS) Globular Cluster Survey (GO-10775) by observing the most accessible 47 of the previous survey’s 65 clusters in three WFC3/UVIS
    Soto, M. et al.

    Advertised on:

    1
    2017
    Bibcode
    2017AJ....153...19S
    Citations
    41