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/

  • Chemical Evolution in the Milky Way: Rotation-based Ages for APOGEE-Kepler Cool Dwarf Stars
    We use models of stellar angular momentum evolution to determine ages for ∼500 stars in the APOGEE-Kepler Cool Dwarfs sample. We focus on lower-main-sequence stars, where other age-dating tools become ineffective. Our age distributions are compared to those derived from asteroseismic and giant samples and solar analogs. We are able to recover
    Claytor, Zachary R. et al.

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    1
    2020
    Citations
    58
  • Carbon, nitrogen, and oxygen abundance gradients in M101 and M31
    We present deep spectrophotometry of 18 H II regions in the nearby massive spiral galaxies M 101 and M 31. We have obtained direct determinations of electron temperature in all the nebulae. We detect the C II 4267 Å line in several H II regions, permitting to derive the radial gradient of C/H in both galaxies. We also determine the radial gradients
    Esteban, C. et al.

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    1
    2020
    Citations
    46
  • Binary Planetary Nebula Central Stars: Validating Kepler/K2 Variability and Amplitudes
    We analyzed the Kepler/K2 Campaign 11 data to validate the periods and amplitudes for the 32 apparently variable central stars of planetary nebulae (PNe) in the sample of 140 PNe in the field. The K2 data yield good values for the periods, but the amplitudes are always too low by up to 10X due to dilution of the photometry from both the nebula and
    Jacoby, G. H. et al.

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    1
    2020
    Citations
    0
  • Are ultra-diffuse galaxies Milky Way-sized?
    Now almost 70 years since its introduction, the effective or half-light radius has become a very popular choice for characterising galaxy size. However, the effective radius measures the concentration of light within galaxies and thus does not capture our intuitive definition of size which is related to the edge or boundary of objects. For this
    Chamba, N. et al.

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    1
    2020
    Citations
    38
  • An ultra-short period rocky super-Earth orbiting the G2-star HD 80653★
    Ultra-short period (USP) planets are a class of exoplanets with periods shorter than one day. The origin of this sub-population of planets is still unclear, with different formation scenarios highly dependent on the composition of the USP planets. A better understanding of this class of exoplanets will, therefore, require an increase in the sample
    Frustagli, G. et al.

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    1
    2020
    Citations
    26
  • Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi
    Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies 1. Although these accreted stellar populations can be forensically identified as kinematically distinct structures within the Galaxy, it is difficult in general to date precisely the age at which any one merger occurred. Recent results have revealed a
    Chaplin, William J. et al.

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    1
    2020
    Citations
    67