Structure in the Dusty Debris Around Vega

Details Structure in the Dusty Debris Around Vega Structure in the Dusty Debris Around Vega

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..324..241w&link_type=abstract

Debris Disks and the Formation of Planets: A Symposium in Memory of Fred Gillett, ASP Conference Series, Vol. 324, Proceedings o

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have made sensitive observations of the Vega system at 1.3 millimeters wavelength with 2'' to 4'' resolution using the IRAM Plateau de Bure interferometer. These data detect the stellar photosphere and two dust emission peaks whose locations may be naturally explained by the dynamical influence of an unseen planet of a few Jupiter masses in a highly eccentric orbit.

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