The structure of the protoplanetary disk surrounding three young intermediate mass stars

200886 citationsJournal Articlegreen Open Access

Authors

D. Fedele · Max Planck Institute for Astronomy

M. E. van den Ancker · European Southern Observatory

B. Acke · KU Leuven

G. van der Plas · European Southern Observatory

R. van Boekel · Max Planck Institute for Astronomy

M. Wittkowski · European Southern Observatory

Th. Henning

Abstract

Aims. We present the first direct comparison of the distribution of the gas, as traced by the [O I] 6300 Å emission, and the dust, as traced by the 10 μm emission, in the planet-forming region of proto-planetary disks around three intermediate-mass stars: HD 101412, HD 135344 B and HD 179218.

Topics & Keywords

Astrophysics and Star Formation Studies Molecular Spectroscopy and Structure Stellar, planetary, and galactic studies

Publication Details

Published in: Astronomy and Astrophysics

Volume 491, Issue 3, pp. 809-820

DOI: 10.1051/0004-6361:200810126

Field-Weighted Citation Impact: 7.09

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The structure of the protoplanetary disk surrounding three young intermediate mass stars

Authors

Abstract

Topics & Keywords

Publication Details