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
    Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set
    We use data from the Gaia DR3 data set to estimate the mass of the Milky Way (MW) by analyzing the rotation curve in the range of distances 5 to 28 kpc. We consider three mass models: The first model adds a spherical dark matter (DM) halo, following the Navarro-Frenk-White (NFW) profile, to the known stellar components. The second model assumes
    Sylos Labini, Francesco et al.

    Fecha de publicación:

    3
    2023
    Bibcode
    2023ApJ...945....3S
    Número de citas
    33
  • Con árbitro
    Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set
    We use data from the Gaia DR3 data set to estimate the mass of the Milky Way (MW) by analyzing the rotation curve in the range of distances 5 to 28 kpc. We consider three mass models: The first model adds a spherical dark matter (DM) halo, following the Navarro-Frenk-White (NFW) profile, to the known stellar components. The second model assumes
    Labini, Francesco Sylos et al.

    Fecha de publicación:

    3
    2023
    Bibcode
    2023ApJ...945....3L
    Número de citas
    0
  • Con árbitro
    MAGIC observations provide compelling evidence of hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7
    Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capable of accelerating cosmic rays (CRs) to ~ PeV energies. However, conclusive observational evidence for this has not yet been found. The SNR G106.3+2.7, detected at 1-100 TeV energies by different γ-ray facilities, is one of the most promising
    MAGIC Collaboration et al.

    Fecha de publicación:

    3
    2023
    Bibcode
    2023A&A...671A..12M
    Número de citas
    24
  • Errata
    Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars (Corrigendum)
    Karinkuzhi, D. et al.

    Fecha de publicación:

    3
    2023
    Bibcode
    2023A&A...671C...8K
    Número de citas
    0
  • Con árbitro
    Jet-induced molecular gas excitation and turbulence in the Teacup
    In order to investigate the impact of radio jets on the interstellar medium (ISM) of galaxies hosting active galactic nuclei (AGN), we present subarcsecond-resolution Atacama Large Millimeter/submillimeter Array (ALMA) CO(2-1) and CO(3-2) observations of the Teacup galaxy. This is a nearby (D L = 388 Mpc) radio-quiet type-2 quasar (QSO2) with a
    Wagner, A. Y. et al.

    Fecha de publicación:

    3
    2023
    Bibcode
    2023A&A...671L..12A
    Número de citas
    40