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Penetration of Interstellar Dust Aggregates Into Circumstellar Dust Disks
Published online by Cambridge University Press: 26 May 2016
Abstract
Interstellar dust particles, which are supposedly aggregates, penetrate dust disks around stars because of the star's motion relative to the surrounding interstellar medium (ISM). We discuss the interrelation of the physical properties of local interstellar dust, the relative motion of the star and the surrounding ISM, and the evolution of the circumstellar disk.
- Type
- Part IV: Protoplanetary and β Pic disks
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- Copyright © Astronomical Society of the Pacific 2004