Gravities and Metallicities of Stars with Protoplanetary Disks

Statistics – Methodology

Scientific paper

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Stars: Pre-Main Sequence, Stars: Absolute Parameters, Stars: Evolution

Scientific paper

We present here the motivation and methodology of an ongoing study of a sample of Herbig Ae/Be and Vega stars surrounded by disks. Stellar gravities and metallicities are computed by comparing the observed spectra with synthetic models. These parameters, together with the effective temperature, will allow us to compute the age and hence, the evolutionary stage of the objects.

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