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

Simple item page
dc.creatorMeyer, Michael R.
dc.creatorBeckwith, Steven V. W.
dc.date2000-01-31
dc.date.accessioned2026-07-07T01:51:59Z
dc.date.available2026-07-07T01:51:59Z
dc.descriptionA 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.
dc.descriptionTo appear in "ISO Surveys of a Dusty Universe", eds. D. Lemke, M. Stickel, & K. Wilke (Heidelberg: Springer-Verlag), in press. 11 postscript pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0001542
dc.identifierhttp://arxiv.org/abs/astro-ph/0001542
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/478
dc.subjectAstrophysics
dc.titleStructure and Evolution of Circumstellar Disks Around Young Stars: New Views from ISO
dc.typetext

Files

Collections

arXiv