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/

  • Refereed
    The connection between mass, environment, and slow rotation in simulated galaxies
    Recent observations from integral field spectroscopy (IFS) indicate that the fraction of galaxies that are slow rotators (SRs), FSR, depends primarily on stellar mass, with no significant dependence on environment. We investigate these trends and the formation paths of SRs using the EAGLE and HYDRANGEA hydrodynamical simulations. EAGLE consists of
    Lagos, Claudia del P. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018MNRAS.476.4327L
    Citations
    84
  • Refereed
    The connection between mass, environment, and slow rotation in simulated galaxies
    Recent observations from integral field spectroscopy (IFS) indicate that the fraction of galaxies that are slow rotators (SRs), FSR, depends primarily on stellar mass, with no significant dependence on environment. We investigate these trends and the formation paths of SRs using the EAGLE and HYDRANGEA hydrodynamical simulations. EAGLE consists of
    del P. Lagos, C. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018MNRAS.476.4327D
  • Refereed
    The CARMENES Search for Exoplanets around M Dwarfs: A Low-mass Planet in the Temperate Zone of the Nearby K2-18
    K2-18 is a nearby M2.5 dwarf, located at 34 pc and hosting a transiting planet that was first discovered by the K2 mission and later confirmed with Spitzer Space Telescope observations. With a radius of ∼2 R ⊕ and an orbital period of ∼33 days, the planet lies in the temperate zone of its host star and receives stellar irradiation similar to that
    Sarkis, P. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018AJ....155..257S
    Citations
    62
  • Refereed
    The CARMENES search for exoplanets around M dwarfs. Radial-velocity variations of active stars in visual-channel spectra
    Context. Previous simulations predicted the activity-induced radial-velocity (RV) variations of M dwarfs to range from 1 cm s-1 to 1 km s-1, depending on various stellar and activity parameters. Aims: We investigate the observed relations between RVs, stellar activity, and stellar parameters of M dwarfs by analyzing CARMENES high-resolution visual
    Tal-Or, L. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018A&A...614A.122T
    Citations
    73
  • Refereed
    Stellar and Planetary Characterization of the Ross 128 Exoplanetary System from APOGEE Spectra
    The first detailed chemical abundance analysis of the M-dwarf (M4.0) exoplanet-hosting star Ross 128 is presented here, based upon near-infrared (1.5–1.7 μm), high-resolution (R ∼ 22,500) spectra from the SDSS Apache Point Galactic Evolution Experiment survey. We determined precise atmospheric parameters T eff = 3231 ± 100 K, log g = 4.96 ± 0.11
    Souto, D. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018ApJ...860L..15S
    Citations
    29
  • Refereed
    Statistics of the polarized submillimetre emission maps from thermal dust in the turbulent, magnetized, diffuse ISM
    Context. The interstellar medium (ISM) is now widely acknowledged to display features ascribable to magnetized turbulence. With the public release of Planck data and the current balloon-borne and ground-based experiments, the growing amount of data tracing the polarized thermal emission from Galactic dust in the submillimetre provides choice
    Levrier, F. et al.

    Advertised on:

    6
    2018
    Bibcode
    2018A&A...614A.124L
    Citations
    15