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/

  • TOI-5005 b: A super-Neptune in the savanna near the ridge
    Context. The Neptunian desert and savanna have recently been found to be separated by a ridge, an overdensity of planets in the period range of ≃3–5 days. These features are thought to be shaped by dynamical and atmospheric processes. However, their roles are not yet well understood. Aims. Our aim was to confirm and characterize the super-Neptune
    Castro-González, A. et al.

    Advertised on:

    11
    2024
    Citations
    0
  • An ultra-short-period super-Earth with an extremely high density and an outer companion
    We present the discovery and characterization of a new multi-planetary system around the Sun-like star K2-360 (EPIC 201595106). K2-360 was first identified in K2 photometry as the host of an ultra-short-period (USP) planet candidate with a period of 0.88 d. We obtained follow-up transit photometry, confirming the star as the host of the signal
    Livingston, John H. et al.

    Advertised on:

    11
    2024
    Citations
    0
  • THE LOCKMAN-SPRESO PROJECT. OPTICAL PROPERTIES OF FAR-INFRARED SELECTED GALAXIES
    Históricamente, los mapas celestes han sido la principal fuente de datos astronómicos, utilizados para explorar y comprender el Universo. Este trabajo está dedicado al estudio de uno de ellos, Lockman-SpReSO, un seguimiento espectroscópico óptico cartográfico de fuentes seleccionadas por su emisión infrarroja, a partir de observaciones previas con
    Mauro González Otero

    Advertised on:

    6
    2024
  • OBSERVATIONAL PROPERTIES OF ACCRETION DISC WINDS IN LOW-MASS X-RAY BINARIES
    Accretion onto compact objects, such as black holes and neutron stars, is one of the most powerful processes in the Universe, involving large exchanges of mass and energy. Among the astrophysical systems where this phenomenon is observed, X-ray binaries are particularly relevant due to their relatively short timescales of evolution, which are
    Mª Guayente Panizo Espinar

    Advertised on:

    7
    2024
  • THREE-DIMENSIONAL RADIATIVE MHD SIMULATIONS OF NEAR-SURFACE CONVECTION IN MAIN SEQUENCE COOL STARS
    This thesis focuses on the study of atmospheres of main sequence cool stars (spectral types G2V, K0V, and M2V, with solar metallicity) by means of three-dimensional time-dependent magneto-hydrodynamic simulations of their near-surface convection and photospheres. The simulations are computed with the MANCHA code, which is adapted to simulate other
    Andrea Perdomo García

    Advertised on:

    7
    2024
  • SPECTROSCOPIC PROPERTIES OF DWARF GALAXIES IN NEARBY CLUSTERS
    Desde el descubrimiento de que existen diferentes tipos de galaxias nos hemos preguntado sobre su formación y evolución. ¿Evolucionan de manera diferente las galaxias de distintos tamaños y masas? Las galaxias gigantes y masivas fueron las primeras en ser estudiadas, su alta luminosidad superficial permitió que los primeros telescopios las
    Jorge Romero Gómez

    Advertised on:

    9
    2024