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/

  • About the multiplicity of M dwarfs
    Stellar multiplicity is a common consequence of the stellar formation process. Low-mass stars are the prime constituent of the nearby stellar population, with late-type accounting for the majority of the hydrogen-fusing objects in the Solar neighborhood. The CARMENES input catalogue of M dwarfs (Carmencita) is a comprehensive and homogeneous sample
    Cifuentes, C. et al.

    Advertised on:

    5
    2023
    Citations
    0
  • A temperate Earth-sized planet with tidal heating transiting an M6 star
    Temperate Earth-sized exoplanets around late-M dwarfs offer a rare opportunity to explore under which conditions planets can develop hospitable climate conditions. The small stellar radius amplifies the atmospheric transit signature, making even compact secondary atmospheres dominated by N 2 or CO 2 amenable to characterization with existing
    Peterson, Merrin S. et al.

    Advertised on:

    5
    2023
    Citations
    14
  • A spectral classification system for hydrogen-deficient carbon stars
    Stellar spectral classification has been highly useful in the study of stars. While there is a currently accepted spectral classification system for carbon stars, the subset of hydrogen-deficient carbon (HdC) stars has not been well described by such a system, due predominantly to their rarity and their variability. Here we present the first system
    Crawford, Courtney L. et al.

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    5
    2023
    Citations
    13
  • A rich molecular chemistry in the gas of the IC 348 star cluster of the Perseus Molecular Cloud
    We present Spitzer 10-34 $\mu{\rm m}$ spectroscopic observations of the diffuse gas in the inner region of the star-forming region IC 348 of the Perseus Molecular Cloud. We find evidence for the strongest mid-IR bands of common molecules as H 2, OH, H 2O, CO 2, and NH 3 and of several carbonaceous molecules which may play an important role in the
    Iglesias-Groth, Susana et al.

    Advertised on:

    5
    2023
    Citations
    4
  • A probability distribution for the amplitude of Solar Cycle 25
    We suggest a method to calculate the probability for the maximum amplitude of Solar Cycle 25 using Bayesian inference. We illustrate this approach with the predictions made by one particular phenomenological model that relates the time interval between termination events of preceding cycles with the amplitude of the next cycle. Our results show
    Arregui, I.

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    5
    2023
    Citations
    0
  • A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
    Dwarf galaxies are excellent cosmological probes, because their shallow potential wells make them very sensitive to the key processes that drive galaxy evolution, including baryonic feedback, tidal interactions, and ram pressure stripping. However, some of the key parameters of dwarf galaxies, which help trace the effects of these processes, are
    Watkins, A. E. et al.

    Advertised on:

    5
    2023
    Citations
    10