Fe b 20 08 The dusty disk around VV

Abstract

We have carried out observations at millimeter and centimeter wavelengths towards VV Ser using the Plateau de Bure Interferometer and the Very Large Array. This allows us to compute the SED from near infrared to centimeter wavelengths. The modeling of the full SED has provided insight into the dust properties and a more accurate value of the disk mass. The… (More)

6 Figures and Tables

Topics

  • Presentations referencing similar topics