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/

  • Thermally altered subsurface material of asteroid (162173) Ryugu
    Analyses of meteorites and theoretical models indicate that some carbonaceous near-Earth asteroids may have been thermally altered due to radiative heating during close approaches to the Sun 1-3. However, the lack of direct measurements on the subsurface doesn't allow us to distinguish thermal alteration due to radiative heating from parent-body
    Kitazato, K. et al.

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    2021
    Citations
    56
  • The GTC gains high spectral resolution
    HORuS, a new high-resolution spectrograph for the Gran Telescopio Canarias, will facilitate an expanded range of optical and near-infrared studies, explains Instrument Scientist Carlos Allende Prieto.
    Allende Prieto, Carlos

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    2021
    Citations
    7
  • Surface Brightness Fluctuations for constraining the chemical enrichment of massive galaxies
    Based on very deep photometry, Surface Brightness Fluctuations (SBF) have been traditionally used to determine galaxy distances. We have recently computed SBF spectra of stellar populations at moderately high resolution, which are fully based on empirical stars. We show that the SBF spectra provide an unprecedented potential for stellar population
    Vazdekis, A. et al.

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    0
    2021
    Citations
    0
  • Signatures of sunspot oscillations and the case for chromospheric resonances
    Sunspots host a large variety of oscillatory phenomena, whose properties depend on the nature of the wave modes and the magnetic and thermodynamic structure of the spot. Umbral chromospheric oscillations exhibit significant differences compared to their photospheric counterparts. They show an enhanced power and a shorter dominant period, from waves
    Felipe, Tobías

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    0
    2021
    Citations
    17
  • Reconstructing the mass accretion histories of nearby red nuggets with their globular cluster systems
    It is generally recognized that massive galaxies form through a combination of in-situ collapse and ex-situ accretion. The in-situ component forms early, where gas collapse and compaction leads to the formation of massive compact systems (blue and red "nuggets") seen at z > 1. The subsequent accretion of satellites brings in ex-situ material
    Beasley, Michael A. et al.

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    0
    2021
    Citations
    1