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/

  • Continuum, CO, and water vapour maps of the Orion Nebula: First millimetre spectral imaging with CONCERTO
    Context. The millimetre spectrum of Galactic regions and galaxies is rich in continuum and molecular lines. This diversity is mostly explored using either broad-band photometry or high-resolution heterodyne spectroscopy. Aims. We aim to map the millimetre continuum emission of Galactic regions with an intermediate spectral resolution between
    Désert, F. -X. et al.

    Advertised on:

    9
    2025
    Citations
    1
  • Chemical abundances and Doppler imaging of the Ap Si/He-wk star HD 100357
    We present the results of time-resolved photometry, abundance analysis, and Doppler imaging of an Ap star, HD 100357. The TESS photometry revealed rotational modulation with a period of 1.6279247 d. Upon inspecting the residuals after removing the rotational period and its harmonics, we found additional frequencies around 15.8054 d $^{-1}$, which
    Dileep, Athul et al.

    Advertised on:

    9
    2025
    Citations
    1
  • Caveats about measuring carbon abundances in stars using the CH band
    Context. Stellar carbon abundances are crucial for tracing the star formation history and predicting the near-infrared emission of galaxies. It is still a complex task to derive accurate carbon abundance estimates for a wide variety of stars because it is hard to measure it based on atomic and molecular lines. It therefore remains challenging to
    Santos-Peral, P. et al.

    Advertised on:

    9
    2025
    Citations
    0
  • Benchmark brown dwarfs – I. A blue M2 + T5 wide binary and a probable young [M4 + M4] + [T7 + T8] hierarchical quadruple
    Benchmark brown dwarfs in wide binary systems are crucial for characterizing substellar objects and calibrating atmospheric and evolutionary models. However, brown dwarf benchmarks with subsolar metallicity, very cool temperatures, or suitability for dynamical mass measurements are rare, limiting our understanding across the full range of mass, age
    Zhang, Z. H. et al.

    Advertised on:

    9
    2025
    Citations
    1
  • Azimuthal offsets in spiral arms of nearby galaxies
    Spiral arms play a central role in disc galaxies, but their dynamical nature remains a long-standing open question. Azimuthal offsets between molecular gas and star formation are expected if gas crosses spiral arms, as predicted by quasi-stationary density wave theory. In this work, we measure offsets between CO and Hα peaks in radial bins for 24
    Querejeta, Miguel et al.

    Advertised on:

    9
    2025
    Citations
    0
  • ATREIDES: I. Embarking on a trek across the exo-Neptunian landscape with the TOI-421 system
    The distribution of close-in exoplanets is shaped by a complex interplay between atmospheric and dynamical processes. The Desert, Ridge, and Savanna (respectively a lack, overoccurence, and mild deficit of Neptunes with increasing periods) illustrate the sensitivity of these worlds to such processes, making them ideal targets to disentangle their
    Bourrier, V. et al.

    Advertised on:

    9
    2025
    Citations
    0