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
    The Tarantula Massive Binary Monitoring. VI. Characterisation of hidden companions in 51 single-lined O-type binaries: A flat mass-ratio distribution and black-hole binary candidates
    Context. Massive binaries hosting a black hole (OB+BH) represent a critical phase in the production of BH mergers in the context of binary evolution. In spite of this, such systems have so far largely avoided detection. Single-lined spectroscopic (SB1) O-type binaries are ideal objects to search for elusive BH companions. Moreover, SB1 binaries
    Shenar, T. et al.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022A&A...665A.148S
    Número de citas
    45
  • Sin árbitro
    The rich chemistry of two warm-giant planets
    High-resolution (HR) ground-based spectrographs have drastically improved the investigation of exoplanet atmospheres. In this scenario the near-infrared (0.9-2.45 μm) HR (R /sim 50000) spectrograph GIANO-B mounted at the Nasmyth-B focus of the Telescopio Nazionale Galileo (TNG) telescope is playing an important role.With the simultaneous detection
    Guilluy, Gloria et al.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022EPSC...16..325G
    Número de citas
    0
  • Con árbitro
    The relic galaxy NGC 1277 rules out intermediate-age stellar populations origin of CO-strong absorptions in massive early-type galaxies
    Massive early-type galaxies (ETGs) show several strong CO absorption features in their H- and K-band spectra that cannot be explained by state-of-the-art stellar population models. For many years, the disagreement has been attributed to the presence of intermediate-age stellar components that are dominated by stars in the asymptotic giant branch
    Eftekhari, Elham et al.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022MNRAS.515L..56E
    Número de citas
    2
  • Sin árbitro
    The planetary system of Proxima Centauri seen with ESPRESSO
    During last decade there have been a tremendous increase in detection and characterization of low-mass exoplanets, reaching the Earth size and mass domain, in particular those orbiting M dwarf stars, due to their smaller sizes and masses, resulting in planet larger transit amplitude and radial velocity signals. Extremely precise instruments such as
    González Hernández, Jonay I.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022EPSC...16.1214G
    Número de citas
    0
  • Sin árbitro
    The Physical Properties of the Near Earth Asteroids 2005 UD and 2001 SG286
    Research into the orbital and physical properties near-Earth asteroids (NEAs) is important as these objects can reveal information about the origin and history of our planetary system.Here we present our findings regarding the physical characteristics of the near Earth asteroids (NEAs) 2005 UD and 2001 SG286. The 2005 UD is currently a possible
    Gherase, Radu et al.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022EPSC...16.1056G
    Número de citas
    0
  • Con árbitro
    The Open Cluster Chemical Abundances and Mapping Survey. VI. Galactic Chemical Gradient Analysis from APOGEE DR17
    The goal of the Open Cluster Chemical Abundances and Mapping (OCCAM) survey is to constrain key Galactic dynamic and chemical evolution parameters by the construction and analysis of a large, comprehensive, uniform data set of infrared spectra for stars in hundreds of open clusters. This sixth contribution from the OCCAM survey presents analysis of
    Myers, Natalie et al.

    Fecha de publicación:

    9
    2022
    Bibcode
    2022AJ....164...85M
    Número de citas
    36