Models of Accretion Disks around Young Stars

Simple item page
dc.creatorD'Alessio, Paola
dc.creatorCalvet, Nuria
dc.creatorHartmann, Lee
dc.creatorMuzerolle, James
dc.creatorSitko, Michael
dc.date2003-09-22
dc.date.accessioned2026-07-07T02:09:42Z
dc.date.available2026-07-07T02:09:42Z
dc.descriptionWe discuss the importance of accretion in calculating disk models for young stellar objects. In particular, we show that a disk inner rim, irradiated by both the star and the accretion shocks at the stellar surface, can naturally explain recent observations of DG Tau with the Keck interferometer. We present models for two objects, with mass accretion rates differing by almost two orders of magnitude, to illustrate the effects of accretion on the overall disk structure and emission.
dc.descriptionTo appear in the Proceeding of IAU Symposium 221, Star Formation at High Angular Resolution, Editors M. Burton, R. Jayawardhana & T. Bourke, Astronomical Society of the Pacific, 8 pages, 1 postscript figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0309590
dc.identifierhttp://arxiv.org/abs/astro-ph/0309590
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6533
dc.subjectAstrophysics
dc.titleModels of Accretion Disks around Young Stars
dc.typetext

Files

Collections

arXiv