Probing Planet Formation Among Nearby Young Stars

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dc.creatorJayawardhana, Ray
dc.date2000-10-02
dc.date.accessioned2026-07-25T17:54:26Z
dc.descriptionThe recent identification of several groups of young stars within 100 parsecs of the Sun has generated widespread interest. Given their proximity and possible age differences, these systems are ideally suited for detailed studies of disk evolution and planet formation. Here I discuss recent results and prospects for the near-future.
dc.description2 pages, to appear in Proceedings of "Star Formation 2000", eds.: O. Kessel-Deynet and A. Burkert
dc.identifierhttps://arxiv.org/abs/astro-ph/0010053
dc.identifierhttp://arxiv.org/abs/astro-ph/0010053
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/51787
dc.subjectAstrophysics
dc.titleProbing Planet Formation Among Nearby Young Stars
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