Transitional disks around young low mass stars

Details Transitional disks around young low mass stars Transitional disks around young low mass stars

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35...33d&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

1

Accretion, Accretion Disks, Infrared: Stars, Planetary Systems: Formation, Planetary Systems: Protoplanetary Disks, Stars: Pre-Main Sequence

Scientific paper

A population of young circumstellar disks have different Spectral Energy Distributions (SEDs) with respect to typical disks, showing a deficit of emission in the near-IR and an excess at mid-IR wavelengths. These SEDs have been interpreted as produced by disks with inner holes, which have been classified as ``Transitional Disks''. These disks are considered the evolutionary link between the full disks typically found around the young T Tauri and Herbig Ae stars, and the debris disks, found around some main sequence stars. In this contribution we summarize the observed/inferred characteristics of these transitional disks and also some of the models proposed to explain their peculiar geometry.

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