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High Angular Resolution Observations of Protostellar Disks

Published online by Cambridge University Press:  19 July 2016

J.-L. Monin ,
J. Bouvier  and
F. Malbet
J.-L. Monin
Affiliation:
Observatoire de Grenoble, Laboratoire d'Astrophysique, 414 rue de la piscine, BP 53X, 38041 Grenoble Cedex, France
J. Bouvier
Affiliation:
Observatoire de Grenoble, Laboratoire d'Astrophysique, 414 rue de la piscine, BP 53X, 38041 Grenoble Cedex, France
F. Malbet
Affiliation:
Observatoire de Grenoble, Laboratoire d'Astrophysique, 414 rue de la piscine, BP 53X, 38041 Grenoble Cedex, France

Abstract

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The existence of circumstellar disks around young stellar objects like T Tauri stars is now well accepted. Such disks would have solar system sizes and, at the distance of the nearest star forming cloud, an angular diameter of 0.01 to 1 arcsecond at most, requiring very high angular resolution to be detected. Due to the nature of the emission process in circumstellar disks and to chromatic properties of ground based observations, disk imaging is expected to be more efficient in the near infrared. Also, multi-aperture interferometry in this wavelength range (1 – 10 μm) is expected to bring considerable insight into the disks properties and evolution in revealing their inner physical structure.

In this paper, we present synthetic images of circumstellar accretion disks. The images have been computed from a complete disk vertical structure model.

Keywords

Young starscircumstellar disksaccretionthermal emissionscatteringimageryinterferometry
Type
Imaging Results: Optical and Infrared
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 387 - 390
Copyright
Copyright © Kluwer 1994 

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