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/

  • CARACTERIZACIÓN ESPECTRAL DE LA SUPERFICIE DEL ASTEROIDE (101955) BENNU A TRAVÉS DEL CONJUNTO INSTRUMENTAL OCAMS DE LA SONDA OSIRIS-REX
    Los asteroides son objetos resultantes de las colisiones y evolución dinámica de los planetesimales originarios del Sistema Solar. Algunos de estos planetesimales originarios —formados en el disco protoplanetario como consecuencia de la agregación de gas y polvo— sobrevivieron al proceso de formación planetaria y permanecen prácticamente
    Juan Luis Rizos García

    Advertised on:

    4
    2020
  • CARACTERIZACIÓN ESPECTRAL DE LA SUPERFICIE DEL ASTEROIDE (101955) BENNU A TRAVÉS DEL CONJUNTO INSTRUMENTAL OCAMS DE LA SONDA OSIRIS-REX
    Los asteroides son objetos resultantes de las colisiones y evolución dinámica de los planetesimales originarios del Sistema Solar. Algunos de estos planetesimales originarios —formados en el disco protoplanetario como consecuencia de la agregación de gas y polvo— sobrevivieron al proceso de formación planetaria y permanecen prácticamente
    Juan Luis Rizos García

    Advertised on:

    4
    2020
  • Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
    Only about 19 Galactic and 25 extragalactic bonafide luminous blue variables (LBVs) are known to date. This incomplete census prevents our understanding of this crucial phase of massive star evolution which leads to the formation of heavy binary black holes via the classical channel. With large samples of LBVs one could better determine the
    Wofford, Aida et al.

    Advertised on:

    4
    2020
    Citations
    12
  • Candidate Brown-dwarf Microlensing Events with Very Short Timescales and Small Angular Einstein Radii
    Short-timescale microlensing events are likely to be produced by substellar brown dwarfs (BDs), but it is difficult to securely identify BD lenses based on only event timescales t E because short-timescale events can also be produced by stellar lenses with high relative lens-source proper motions. In this paper, we report three strong candidate BD
    Han, Cheongho et al.

    Advertised on:

    4
    2020
    Citations
    16
  • Analysis of the galaxy size versus stellar mass relation
    The scatter in the galaxy size versus stellar mass (M ⋆) relation gets largely reduced when, rather than the half-mass radius R e, the size at a fixed surface density is used. Here, we address why this happens. We show how a reduction is to be expected because any two galaxies with the same M ⋆ have at least one radius with identical surface
    Sánchez Almeida, J.

    Advertised on:

    4
    2020
    Citations
    23
  • An artificial impact on the asteroid (162173) Ryugu formed a crater in the gravity-dominated regime
    The Hayabusa2 spacecraft investigated the small asteroid Ryugu, which has a rubble-pile structure. We describe an impact experiment on Ryugu using Hayabusa2’s Small Carry-on Impactor. The impact produced an artificial crater with a diameter >10 meters, which has a semicircular shape, an elevated rim, and a central pit. Images of the impact and
    Arakawa, M. et al.

    Advertised on:

    4
    2020
    Citations
    222