Journal
ASTROPHYSICAL JOURNAL
Volume 650, Issue 1, Pages L83-L86Publisher
IOP PUBLISHING LTD
DOI: 10.1086/508707
Keywords
circumstellar matter; planetary systems : protoplanetary disks; stars : formation
Categories
Ask authors/readers for more resources
We present 24 mm 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 mm 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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available