Publicaciones

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  • Mineralogical and photometric analysis of V-type asteroids
    Most of the V-types that are known are located in the inner main belt and are members of the Vesta collisional family. The analysis of the photometric and spectroscopic properties of asteroids inside and outside the Vesta family, including V-types in the middle and outer main belt, can answer questions about the existence of differentiated bodies
    Medeiros, H. et al.

    Fecha de publicación:

    9
    2018
    Número de citas
    0
  • Mineralogical characterization of some basaltic asteroids in the neighborhood of (4) Vesta: first results
    We present reflectance spectra of 19 V-type asteroids obtained at the 3.6 m Telescopio Nazionale Galileo covering 0.8 to 2.5 μm. For 8 of these asteroids we obtained also visible spectra in the same observational run. The range from 0.8 to 2.5 μm, encompassing the 1 and 2 μm pyroxene features, allows a precise mineralogical characterization of
    Carvano, Jorge M. et al.

    Fecha de publicación:

    9
    2004
    Número de citas
    63