Spitzer MIPS 24 μm Detection of Photoevaporating Protoplanetary Disks

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Published 2006 September 25 © 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Zoltan Balog et al 2006 ApJ 650 L83 DOI 10.1086/508707

1538-4357/650/1/L83

Abstract

We present 24 μm images of three protoplanetary disks being photoevaporated around high-mass O-type stars. These objects have "cometary" structure where the dust pulled away from the disk by the photoevaporating flow is forced away from the O star by photon pressure on the dust and heating and ionization of the gas. Models of the 24 and 8 μm brightness profiles agree with this hypothesis. These models show that the mass-loss rate needed to sustain such a configuration is in agreement with or somewhat less than the theoretical predictions for the photoevaporation process.

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10.1086/508707