Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Con árbitro
    Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model
    Context. Recent results for asteroid rotation periods from the TESS mission showed how strongly previous studies have underestimated the number of slow rotators, revealing the importance of studying those targets. For most slowly rotating asteroids (those with P > 12 h), no spin and shape model is available because of observation selection effects
    Marciniak, A. et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021A&A...654A..87M
    Número de citas
    13
  • Con árbitro
    Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
    Supriya, Hebbur Dayananda et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021ApJ...920..140S
    Número de citas
    8
  • Con árbitro
    Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
    The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the extended solar atmosphere requires modeling the polarization of forbidden and permitted coronal lines. To this end, it is important to develop efficient codes to calculate the Stokes profiles
    Hebbur Dayananda, Supriya et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021ApJ...920..140H
    Número de citas
    0
  • Sin árbitro
    Physical properties of the cubewano 19521 Chaos from a multi-chord stellar occultation
    Trans-Neptunian Objects (TNOs) have had an increasing interest since the discovery of (15760) Albion in 1992. These objects are considered remnants of the Solar System formation, and can thus provide clues about its origin and evolution. One of the best techniques to study TNOs from ground-based telescopes are stellar occultations which, if
    Vara-Lubiano, Mónica et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021DPS....5330711V
    Número de citas
    0
  • Sin árbitro
    Physical properties of Hi'iaka from stellar occultation data
    Two very bright stellar occultations by Hi'iaka, the largest satellite of the dwarf planet Haumea, were predicted to take place during in April 2021. Since the uncertainty on Hi'iaka's shadow path was large due to uncertainty on Hi'iaka's position with respect to Haumea, we performed an observational campaign using medium-sized telescopes to obtain
    Fernández-Valenzuela, Estela et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021DPS....5350305F
    Número de citas
    0
  • Sin árbitro
    Physical properties of 5 near-Earth asteroids observed with the Arecibo Planetary Radar within NEOROCKS project.
    The near-Earth object (NEO) population is composed of asteroids and comets that have orbits close to the Earth. This vicinity to the Earth gives us some advantages, because this population is the most accessible vestige from the building blocks that formed the Solar System, for spacecrafts, and for detailed observations from ground-based facilities
    Medeiros, Hissa et al.

    Fecha de publicación:

    10
    2021
    Bibcode
    2021DPS....5330301M
    Número de citas
    0