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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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31 Dec 1999 | | Subject: | astro-ph | | Affiliation: | Steward Observatory, The University of Arizona) Steven V.W. Beckwith (Space Telescope Science Institute | | 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. | | Source: | arXiv, astro-ph/0001542 | | Services: | Forum | Review | PDF | Favorites | |
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