Spitzer MIPS 24 μm detection of photoevaporating protoplanetary disks

Zoltan Balog, G. H. Rieke, Kate Y.L. Su, James Muzerolle, Erick T. Young

Research output: Contribution to journalArticlepeer-review

24 Scopus citations


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.

Original languageEnglish (US)
Pages (from-to)L83-L86
JournalAstrophysical Journal
Issue number1 II
StatePublished - Oct 10 2006


  • Circumstellar matter
  • Planetary systems: protoplanetary disks
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science


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