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/

  • Quantitative Spectroscopic Analysis of O stars in the IACOB+OWN project: Massive stars in the Galaxy with GAIA-DR3
    Massive stars are luminous beacons that help us to extract information about the star formation history and the chemodynamical evolution of galaxies in the Universe. Our Galaxy is full of massive stars, which expend their short-lived existence within bright star-forming regions, depositing huge amounts of mechanical and radiative energy to the
    Holgado, G. et al.

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    5
    2023
    Citations
    0
  • Reconstructing the optical spectral variability of gamma-ray blazars
    Blazars are a subclass of active galactic nuclei (AGNs) with a relativistically boosted jet pointing towards the Earth. They are one of the most violent and variable objects in the Universe, showing extreme variability across the entire electromagnetic spectrum. The jet generally dominates the optical emission of these sources. However, other
    Otero-Santos, J. et al.

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    5
    2023
    Citations
    0
  • Resolving the ionised outflows in GATOS Seyfert galaxies with GTC/MEGARA
    Active galactic nuclei (AGNs) play a crucial role in galaxy evolution, as their feedback has been proposed to shape some galaxy properties (for instance, the galaxy luminosity functions). Ionised outflows and their feedback effects have been routinely studied in powerful AGNs, but are less explored for Seyfert galaxies. The abundance of the latter
    Peralta de Arriba, L. et al.

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    5
    2023
    Citations
    0
  • Searching for a second occultation in EPIC 204376071
    EPIC 204376071 is a young ($\sim$10 Myr) M star (estimated mass 0.16 M$_\odot$, and radius 0.63 R$_\odot$), probable member of the Upper Sco association, that exhibited an 80% drop in flux lasting one day, in the course of one campaign of the K2 mission (Rappaport et al. 2019). Different scenarios have been proposed to explain this feature, some of
    Alonso, Roi et al.

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    5
    2023
    Citations
    0
  • Strong lithium lines in red supergiants at different metallicities
    Lithium (Li) is a fragile material, easily destroyed in stellar interiors. Within our current understanding of stellar evolution for stars more massive than $\sim6\:$M$_{\odot}$, Li should be depleted in the atmospheres of all such stars well before the time when they reach the He core burning phase. Despite this prediction, we find a high fraction
    Negueruela, I. et al.

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    5
    2023
    Citations
    0
  • The blue supergiant 2MASS J20395358+4222505, a Rosetta stone in the realm of massive stars
    2MASS J20395358+4222505 is a highly extincted (Av= 9.6 mag) early B-supergiant located in the nearest massive star forming region, Cyg-X, in the outskirts of the massive star association Cyg OB2. A mass of M= 46 M$_\odot$ and a luminosity of log(L/L$_\odot$)= 5.7 make it one of the most massive and luminous stars in the Milky Way. Interestingly
    Herrero, A. et al.

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    5
    2023
    Citations
    0