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/

  • Understanding the thermal and magnetic properties of an X-class flare in the low solar atmosphere
    Recently, the exploitation of spectropolarimetric data has allowed to improve our knowledge of the dynamical and magnetic response of the photospheric and chromospheric layers to the rapid release of energy occurring during solar flares. In this framework, we have used high-resolution observations acquired on 22nd October 2014 during an X1.6
    Ferrente, Fabiana et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Unveiling galaxy protoclusters in the era of Euclid
    How large-scale structures formed in the early universe is a key cosmological question with few answers from empirical evidence. Unveiling galaxy clusters and their high-z progenitors (i.e., protoclusters) is essential to picture galaxy evolution drawn by the hierarchical formation scenario. However, unveiling these early structures at high
    Ramos Chernenko, Nataliya et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Unveiling the central kpc of Type I AGN host galaxies in seeing-limited IFS data
    The evolution of galaxies appears linked to the growth of supermassive black holes (SMBH), as evidenced by empirical scale relations between hosts' large-scale properties and the mass of their central black holes. This co-evolutionary scenario suggests that all galaxies experience nuclear activity — active phases during which the black hole
    García Lorenzo, Begoña et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Using gas kinematics to measure resonant structures in disc galaxies: the interaction of M51 with NGC 5195
    Interstellar gas offers advantages when quantifying the structure of the resonances in disc galaxies. The gas is concentrated close to the disc mid-plane, making it easier to determine its in-plane velocity components, and it offers sharp emission lines for good velocity resolution. These properties are shared by atomic, molecular, and ionized gas
    Beckman, John et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Witnessing the rapid growth of disk galaxies over cosmic time
    The Hubble and James Webb Space Telescopes, with their outstanding depth and spatial resolution, are opening up the possibility of studying the edges of disk galaxies over a significant cosmic time interval. This allows us to study in detail the evolution of galaxy edges over the past 8 Gyr. The edge of galaxies, understood here as the farthest
    Raji, Samane et al.

    Advertised on:

    7
    2024
    Citations
    0
  • A Survey of Protoplanetary Disks Using the Keck/NIRC2 Vortex Coronagraph
    Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations of protoplanetary disks in the millimeter continuum have shown a variety of radial gaps, cavities, and spiral features. These substructures may be signposts for ongoing planet formation, and therefore these systems are promising targets for direct imaging planet searches in the
    Wallack, Nicole L. et al.

    Advertised on:

    8
    2024
    Citations
    0