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Structure and Evolution of Circumstellar Disks Around Young Stars: New Views from ISO

Michael R. Meyer·Steven V. W. Beckwith
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Abstract

A question central to understanding the origin of our solar system is: how do planets form in circumstellar disks around young stars? Because of the complex nature of the physical processes involved, multi-wavelength observations of large samples will be required in order to obtain a complete answer to this question. Surveys undertaken with ISO have helped to solve pieces of this puzzle in addition to uncovering new mysteries. We review a variety of studies aimed at understanding; i) the physical structure and composition of circumstellar disks commonly found surrounding young stellar objects; and ii) the evolution of circumstellar disks from the active accretion phase to post-planet building debris disks.

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Michael R. Meyer, Steven V. W. Beckwith. 2000-01-31. Structure and Evolution of Circumstellar Disks Around Young Stars: New Views from ISO. https://arxiv.org/abs/astro-ph/0001542

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