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Observational Evidence for Grain Growth
DOI: 10.1007/s11038-010-9374-z
Bibcode: 2011EM&P..108...45M
Meeus, Gwendolyn
Discs around young stars are the sites of planet formation. The first step in this process is the growth of submicron grains to larger sized grains. I will review evidence for dust growth in CS discs, based on ISO and Spitzer infrared spectroscopic observations. Intermediate-mass stars, solar-type stars and even brown dwarfs will be discussed in t…
2011
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Earth Moon and Planets
ISO
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