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A Quantitative Study of Limb Darkening in Accretion Disks

Published online by Cambridge University Press:  12 April 2016

M. P. Diaz ,
R. A. Wade  and
I. Hubeny
M. P. Diaz
Affiliation:
Department of Astronomy, Pennsylvania State University, University Park, PA 16802, USA
R. A. Wade
Affiliation:
Department of Astronomy, Pennsylvania State University, University Park, PA 16802, USA
I. Hubeny
Affiliation:
Goddard Space Flight Center, Greenbelt, MD 20771, USA

Abstract

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The UV emission of accretion disks was synthesized for a grid of optically thick models that cover the high-Ṁ nova-like regime, aiming to quantify the effect of limb darkening in the integrated and radially resolved spectrum of the disk.

Type
Accretion Discs
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 123 - 124
Copyright
Copyright © Kluwer 1996

References

Hubeny, I., 1990, Ap. J., 351, 632 Google Scholar
Hubeny, I., Lanz, T., Jefferys, C.S., 1994, Collaborative Computational Project 7, 20, 30 Google Scholar
Kriz, S., Hubeny, I., 1986, Bull. Ast. Inst. Czech. 37, 129 Google Scholar
Kurucz, R.L., 1990, Trans IAU 20B, 169 Google Scholar
Wade, R.A., Rucinski, S.M., 1985, A&AS, 60, 471 Google Scholar