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Models of Accretion Disks Around Young Stars

Published online by Cambridge University Press:  23 September 2016

Paola D'Alessio ,
Nuria Calvet ,
Lee Hartmann ,
James Muzerolle  and
Michael Sitko
Paola D'Alessio
Affiliation:
Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Ap. Postal 3-72, Morelia, Michoacan, México
Nuria Calvet
Affiliation:
Smithsonian Astrophysical Observatory, 60 Garden Street, MS 42, Cambridge, MA 02138
Lee Hartmann
Affiliation:
Smithsonian Astrophysical Observatory, 60 Garden Street, MS 42, Cambridge, MA 02138
James Muzerolle
Affiliation:
Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721
Michael Sitko
Affiliation:
Department of Physics, University of Cincinnati, Cincinnati, OH 45221-0011

Abstract

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We 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.

Type
Part 8: Disks
Information
Symposium - International Astronomical Union , Volume 221: Star Formation at High Angular Resolution , 2004 , pp. 403 - 410
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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