Dynamics of the dust material surrounding VEGA
The spectrum corresponding to the emission of radiation from a dust distribution dominated by the dynamical action of the Poynting Robertson Effect is discussed and a model is applied to the dust surrounding Vega. It is found that a dust cloud extending from 41 to 177 AU match the 25, 60 and 100 micron measurements from IRAS. The 193 micron data
Buitrago, J. et al.
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1985