The Dusty Disk around VV Serpens

  title={The Dusty Disk around VV Serpens},
  author={Tom'as Alonso-Albi and Asunci{\'o}n Fuente and Rafael Bachiller and Roberto Neri and Pere Planesas and Leonardo Testi},
  journal={The Astrophysical Journal},
  pages={1289 - 1294}
We have carried out observations at millimeter and centimeter wavelengths toward 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 mass of dust in the disk around VV Ser is found to be about 4 × 10−5 M☉, i.e., 400 times larger than previous estimates. Moreover, the SED… 

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