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/

  • 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.

    Advertised on:

    3
    2017
    Citations
    32
  • 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.

    Advertised on:

    3
    2017
    Citations
    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.

    Advertised on:

    3
    2017
    Citations
    7
  • 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.

    Advertised on:

    3
    2017
    Citations
    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.

    Advertised on:

    3
    2017
    Citations
    26
  • 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.

    Advertised on:

    3
    2017
    Citations
    103