Observational Evidence for Grain Growth

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 s...

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Veröffentlicht in:	Earth, moon, and planets moon, and planets, 2011-05, Vol.108 (1), p.45-50
1. Verfasser:	Meeus, Gwendolyn
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astronomy Astrophysics and Astroparticles Celestial bodies Cosmic dust Discs Disks Dust Evolution Grain growth Grains Infrared imaging systems Infrared spectroscopy Observations and Techniques Physics Physics and Astronomy Planet formation Planetology Planets Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spectroscopic observation Spectroscopy Star & galaxy formation Star formation Stars Stars & galaxies Stellar evolution
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