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We show that non-magnetic models for the evolution of pre-main-sequence (PMS) stars cannot simultaneously describe the colour-magnitude diagram (CMD) and the pattern of lithium depletion seen in the cluster of young, low-mass stars surrounding gamma(2) Velorum. The age of 7.5 +/- 1 Myr inferred f...


Jeffries, RDJackson, RJFranciosini, ERandich, SBarrado, DFrasca, AKlutsch, ALanzafame, ACPrisinzano, LSacco, GGGilmore, GVallenari, AAlfaro, EJKoposov, SEPancino, EBayo, ACasey, ARCostado, MTDamiani, FHourihane, ALewis, JJofre, PMagrini, LMonaco, LMorbidelli, LWorley, CCZaggia, SZwitter, T[The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars]The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars

Bright features have been recently discovered by Dawn on Ceres, which extend previous photometric and Space Telescope observations. These features should produce distortions of the line profiles of the reflected solar spectrum and therefore an apparent radial velocity variation modulated by the r...


Molaro, PLanza, AFMonaco, LTosi, FLo Curto, GFulle, MPasquini, L[Daily variability of Ceres’ albedo detected by means of radial velocities changes of the reflected sunlight]Daily variability of Ceres’ albedo detected by means of radial velocities changes of the reflected sunlight

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