Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • JWST Observations of the Ring Nebula (NGC 6720). III. A Dusty Disk around Its Central Star
    The planetary nebula NGC 6720, also known as the "Ring Nebula," is one of the most iconic examples of nearby planetary nebulae whose morphologies present a challenge to our theoretical understanding of the processes that govern the deaths of most stars in the Universe that evolve on a Hubble time. We present new imaging with JWST of the central
    Sahai, Raghvendra et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    1
  • TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star
    We report the discovery of TOI-3493 b, a sub-Neptune-sized planet on an 8.15-d orbit transiting the bright (V=9.3) G0 star HD 119355 (aka TIC 203377303) initially identified by NASA's TESS space mission. With the aim of confirming the planetary nature of the transit signal detected by TESS and determining the mass of the planet, we performed an
    Chaturvedi, P. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • The Sunrise Ultraviolet Spectropolarimeter and Imager: Instrument Description
    The third science flight of the balloon-borne solar observatory SUNRISE carries three entirely new post-focus science instruments with spectropolarimetric capabilities, concurrently covering an extended spectral range from the near ultraviolet to the near infrared. Sampling a larger height range, from the low photosphere to the chromosphere, with
    Feller, Alex et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • MaNGA AGN dwarf galaxies (MAD): II. AGN outflows in dwarf galaxies
    Context. Feedback from an active galactic nucleus (AGN) is one of the most important mechanisms in galaxy evolution. This phenomenon is usually found in massive galaxies and is known to regulate star formation. Although dwarf galaxies are assumed to be regulated by supernova feedback, recent studies have offered evidence to support the presence of
    Rodríguez Morales, V. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    1
  • Chlorine abundances in star-forming regions of the local Universe
    Aims. We aim to study the behaviour of Cl abundance and its ratios with respect to O, S, and Ar abundances in a sample of more than 200 spectra of Galactic and extragalactic H II regions and star-forming galaxies (SFGs) of the local Universe. Methods. We used the DEep Spectra of Ionised REgions Database (DESIRED) Extended project (DESIRED-E) that
    Orte-García, M. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • On the chlorine abundance in H II regions
    Chlorine (Cl) is a chemical element of the group of the halogens and is between the 17th and the 20th most abundant elements in the Solar System. It is thought to be produced from the capture of a proton or neutron by specific alpha-element isotopes during both hydrostatic and explosive oxygen burning, though some contribution may come from Type Ia
    Orte-García, M. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0