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/

  • Measurement of the B± Meson Nuclear Modification Factor in Pb-Pb Collisions at √{sN N }=5.02 TeV
    The differential production cross sections of B± mesons are measured via the exclusive decay channels B±→J /ψ K±→μ+μ-K± as a function of transverse momentum in p p and Pb-Pb collisions at a center-of-mass energy √{sN N }=5.02 TeV per nucleon pair with the CMS detector at the LHC. The p p (Pb-Pb ) data set used for this analysis corresponds to an
    Sirunyan, A. M. et al.

    Advertised on:

    10
    2017
    Citations
    67
  • Mass-metallicity relation of dwarf galaxies and its dependency on time: clues from resolved systems and comparison with massive galaxies
    Aims: We present a new approach to study the mass-metallicity relation and its dependency on time. Methods: We used the star formation history (SFH) derived from color-magnitude diagram fitting techniques of a sample of Local Group (LG) dwarfs to obtain stellar masses, metallicities, and star-formation rates (SFR) to analyze the mass-metallicity
    Hidalgo, S. L.

    Advertised on:

    10
    2017
    Citations
    23
  • Magnetic topological analysis of coronal bright points
    Context. We report on the first of a series of studies on coronal bright points which investigate the physical mechanism that generates these phenomena. Aims: The aim of this paper is to understand the magnetic-field structure that hosts the bright points. Methods: We use longitudinal magnetograms taken by the Solar Optical Telescope with the
    Galsgaard, K. et al.

    Advertised on:

    10
    2017
    Citations
    19
  • MAGIC observations of the microquasar V404 Cygni during the 2015 outburst
    The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15-31, during which its flux in hard X-rays (20-40 keV) reached about 40 times the Crab nebula flux. Because of the exceptional interest of the flaring activity from this source, observations at several wavelengths were conducted. The MAGIC telescopes, triggered by the
    Ahnen, M. L. et al.

    Advertised on:

    10
    2017
    Citations
    9
  • Imaging the elusive H-poor gas in planetary nebulae with large abundance discrepancy factors
    The discrepancy between abundances computed using optical recombination lines (ORLs) and collisionally excited lines (CELs) is a major, unresolved problem with significant implications for the determination of chemical abundances throughout the Universe. In planetary nebulae (PNe), the most common explanation for the discrepancy is that two
    García-Rojas, J. et al.

    Advertised on:

    10
    2017
    Citations
    10
  • Hunting for binary central stars of planetary nebulae: exploiting archival data
    The detection of new binary central stars of planetary nebulae is crucial to definitively determine the importance of binary interactions in the nebular morphology. In this context, we are working on a project that aims to increase the low number of binary central stars detected so far. For that, we are first analyzing public archival data in order
    Aller, A. et al.

    Advertised on:

    10
    2017
    Citations
    0