Tipo de publicación: Sin árbitro

  • Publicación
    The SED of Low-Luminosity AGNs at high-spatial resolution
    The inner structure of AGNs is expected to change below a certain luminosity limit. The big blue bump, footprint of the accretion disk, is absent for the...
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    The seismic structure of the Sun from GONG
    Not Available
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    The Seismology Programme of CoRoT
    We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the...
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    The Sensitivity of the Second Solar Spectrum of the Li I 6708 Å Doublet to the Lithium Isotopic Abundance and to a Microturbulent Magnetic Field
    The second solar spectrum offers a novel diagnostic window not only to explore the magnetic field of our nearest star, but also to determine the atomic and...
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    The separated star formation main sequence of bulges and discs. New clues for the galaxy mass assembly
    Disc galaxies are complex systems shaped by different stellar structures such as bulges, discs, and bars. Every galaxy structure keeps a unique memory of their...
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    The Seyfert Nucleus in the SO Galaxy NGC 5252
    Not Available
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    The Shape of Extremely Metal-Poor Galaxies
    This work is the first study on the 3D shape of starbursting extremely metal-poor galaxies (XMPs; a galaxy is said to be an XMP if its ionized gas-phase...
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    The Shape of III Zw2 Hα Line: Evidence of Keplerian Relativistic Disk
    We have analyzed the shape of III Zw2 Hα emission line observed at Isaac Newton telescope. A model with a Keplerian relativistic disk plus one emission region...
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    The shape of the Galactic abundance gradient of oxygen from deep spectra of H II regions
    We present results of an ongoing project dedicated to reassess the shape of the radial abundance gradient of O in the Milky Way based on deep spectroscopy of H...