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/

  • Inferring planetary obliquity using rotational and orbital photometry
    The obliquity of a terrestrial planet is an important clue about its formation and critical to its climate. Previous studies using simulated photometry of Earth show that continuous observations over most of a planet's orbit can be inverted to infer obliquity. However, few studies of more general planets with arbitrary albedo markings have been
    Schwartz, J. C. et al.

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    3
    2016
    Citations
    40
  • Heating of the Partially Ionized Solar Chromosphere by Waves in Magnetic Structures
    In this paper, we show a “proof of concept” of the heating mechanism of the solar chromosphere due to wave dissipation caused by the effects of partial ionization. Numerical modeling of non-linear wave propagation in a magnetic flux tube, embedded in the solar atmosphere, is performed by solving a system of single-fluid quasi-MHD equations, which
    Shelyag, S. et al.

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    3
    2016
    Citations
    58
  • Erratum: “Results of a Search for γ Dor and δ Sct Stars with the Kepler Spacecraft” (2015, AJ, 149, 68)
    Not Available
    Jackiewicz, J. et al.

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    3
    2016
    Citations
    1
  • Early-type dwarf galaxies with multicomponent stellar structure: Are they remnants of disc galaxies strongly transformed by their environment?
    Context. The surface brightness distribution of ~30-40% of the early-type dwarf galaxies with - 18 ≤ MB ≤ -15 in the Virgo and the Coma clusters is fitted by models that include two structural components (Sérsic + exponential) as for bright disc galaxies. Aims: The goal of the present study is to determine whether early-type dwarf galaxies with a
    Aguerri, J. A. L.

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    3
    2016
    Citations
    11
  • Dust properties of Lyman-break galaxies at z ~ 3
    Context. Since the mid-1990s, the sample of Lyman-break galaxies (LBGs) has been growing thanks to the increasing sensitivities in the optical and in near-infrared telescopes for objects at z> 2.5. However, the dust properties of the LBGs are poorly known because the samples are small and/or biased against far-infrared (far-IR) or submillimeter
    Álvarez-Márquez, J. et al.

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    3
    2016
    Citations
    76