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Penetration of Interstellar Dust Aggregates Into Circumstellar Dust Disks

Published online by Cambridge University Press:  26 May 2016

Hiroshi Kimura  and
Ingrid Mann
Hiroshi Kimura
Affiliation:
Institut für Planetologie, Westfälische Wilhelms-Universität, Wilhelm-Klemm-Straβe 10, D-48149 Münster, Germany
Ingrid Mann
Affiliation:
Space Science Department ESTEC SCI-SO, PO Bus 299, 220 AG Noordwijk, The Netherlands

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 347 - 349
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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