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Interferometric Observations of Disks around PMS Binary Stars

Published online by Cambridge University Press:  13 May 2016

Anne Dutrey
Anne Dutrey*
Affiliation:
Institut de Radio Astronomie Millimétrique 300 rue de la picine, F-38406, Saint-Martin-d'Hères, France

Abstract

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Current millimetre arrays are well suited to study the gas and dust distribution around young binary systems of separation ∼ 0.3–3″. In particular, they clearly demonstrate that disks around binary systems are tidally truncated. I review here the observed properties at mm wavelengths of the gas and dust around the best known multiple systems. I also discuss the limitations of current mm interferometers.

Type
VII. Environments of Young Binaries - Direct Imaging
Information
Symposium - International Astronomical Union , Volume 200: The Formation of Binary Stars , 2001 , pp. 219 - 228
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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