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MW94

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SIRTF observations can diagnose structure & composition of flared disks around solar-type stars. What are the Conditions. Under which Planets Form? ... – PowerPoint PPT presentation

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Title: MW94


1
What are the Conditions Under which Planets Form?
(Chiang and Goldreich)
Predicted Spectrum (star plus disk)
HST Image
Total
33
Stellar
32
log Ln (erg s-1)
31
Surface
30
29
Interior
1
10
100
1000
Star
Wavelength (mm)
SIRTF observations can diagnose structure
composition of flared disks around solar-type
stars
Model disk with flared surface
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