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The formation of stars and planets

The formation of stars and planets. Day 3, Topic 3: Irradiated protoplanetary disks Lecture by: C.P. Dullemond. This is because energy is:. Spectral Energy Distributions (SEDs). Plotting normal flux makes it look as if the source emits much more infrared radiation than optical radiation:.

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Disk loses opacity - PowerPoint PPT Presentation

The formation of stars and planets