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

  • The Splitting of Double-component Active Asteroid P/2016 J1 (PANSTARRS)
    We present deep imaging observations, orbital dynamics, and dust-tail model analyses of the double-component asteroid P/2016 J1 (J1-A and J1-B). The observations were acquired at the Gran Telescopio Canarias (GTC) and the Canada–France–Hawaii Telescope (CFHT) from mid-March to late July of 2016. A statistical analysis of backward-in-time
    Moreno, F. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    31
  • The Rb problem in massive AGB stars.
    The asymptotic giant branch (AGB) is formed by low- and intermediate-mass stars (0.8 M_{⊙} M 8 M_{⊙}) in their last nuclear-burning phase, when they develop thermal pulses (TP) and suffer extreme mass loss. AGB stars are the main contributor to the enrichment of the interstellar medium (ISM) and thus to the chemical evolution of galaxies. In
    Pérez-Mesa, V. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    0
  • The QUIJOTE experiment: project status and first scientific results
    We present the current status of the QUIJOTE (Q-U-I JOint TEnerife) experiment, a new polarimeter with the aim of characterizing the polarization of the Cosmic Microwave Background, and other galactic or extra-galactic physical processes that emit in microwaves in the frequency range 10-42 GHz, and at largeangular scales (around 1 degree resolution
    Rubiño-Martín, J. A. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    6
  • The OCCASO survey
    Open clusters (OCs) are crucial for studying the formation and evolution of the Galactic disc. The lack of a large number of OCs analysed homogeneously hampers the investigations. The OCCASO survey provides homogeneous radial velocities, physical parameters and individual chemical abundances from high-resolution spectroscopy. We present the
    Casamiquela, L. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    0
  • The molecular gas mass of M 33
    Do some environments favor efficient conversion of molecular gas into stars? To answer this, we need to be able to estimate the H2 mass. Traditionally, this is done using CO observations and a few assumptions but the Herschel observations which cover the far-IR dust spectrum make it possible to estimate the molecular gas mass independently of CO
    Gratier, P. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    24
  • The ISLAandS Project II: The Lifetime Star-formation Histories of Six Andomeda DSPHS
    The Initial Star formation and Lifetimes of Andromeda Satellites (ISLAndS) project employs Hubble Space Telescope imaging to study a representative sample of six Andromeda dSph satellite companion galaxies. Our main goal is to determine whether the star formation histories (SFHs) of the Andromeda dSph satellites demonstrate significant statistical
    Skillman, E. D. et al.

    Fecha de publicación:

    3
    2017
    Número de citas
    92