Tipo de publicación: Sin árbitro

  • Publicación
    Spatially resolved molecular gas in early-type galaxies
    In around ~25% of early-type galaxies (ETGs) UV emission from young stellar populations is present. Molecular gas reservoirs have been detected in these systems...
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    Spatially Resolved Spectral Energy Distributions of Nearby Galaxies
    We present azimuthally-averaged spectral energy distributions (SEDs) from FUV to FIR, as a function of radius, for the galaxies included in the SINGS sample...
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    Spatially Resolved Spectroscopy and Imaging of the H II Galaxy II ZW 33
    Preliminary results from spatially resolved spectroscopy and photometry of the star-forming dwarf galaxy II Zw 33 are presented. Our study has revealed the...
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    Spatially Resolved Star Formation Main Sequence of Galaxies
    The relation known as Star Formation Main Sequence (SFMS) of galaxies is defined in terms of stellar mass and star formation rate. This approximately linear...
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    Spatially resolved star-formation in nearby early-type galaxies
    Not Available
  • Publicación
    Spatially Resolved Stellar Populations in Dwarf and Giant Galaxies
    The dwarf elliptical galaxies (dEs) are more luminous than dwarf spheroidals and fainter than "normal" ellipticals. In this paper I investigate the...
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    Spatially Resolved Studies of DIBs in Galaxies outside the Local Group
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    Spatially Resolving the Inner Gaseous Disc of the Herbig Star 51 Oph through its CO Ro-vibration Emission
    Near-infrared interferometry gives us the opportunity to spatially resolve the circumstellar environment of young stars at sub-astronomical-unit (au) scales...
  • Publicación
    Spatially Resolving the Quasar Broad Emission Line Region
    The angular resolution of the Very Large Telescope Interferometer (VLTI) and the excellent sensitivity of GRAVITY have led to the first detection of spatially...