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