Numerical radiative transfer in Be disks - Ph.D. Thesis, Northwestern University

Research output: Other contribution

Abstract

The ionization structure of a gaseous disk rotating around a central Be star in circular, Keplerian orbits is computed, and the profiles of emission lines from the disk studied. Three cases are considered, each modeled on the observations of the shell sta
Original languageEnglish
StatePublished - 1983

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theses
circular orbits
rotating disks
radiative transfer
stars
ionization
profiles

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@misc{73003d5f4f0a4262b48390aa7b132b45,
title = "Numerical radiative transfer in Be disks - Ph.D. Thesis, Northwestern University",
abstract = "The ionization structure of a gaseous disk rotating around a central Be star in circular, Keplerian orbits is computed, and the profiles of emission lines from the disk studied. Three cases are considered, each modeled on the observations of the shell sta",
author = "D.A. Brown",
year = "1983",
language = "English",
type = "Other",

}

TY - GEN

T1 - Numerical radiative transfer in Be disks - Ph.D. Thesis, Northwestern University

AU - Brown, D.A.

PY - 1983

Y1 - 1983

N2 - The ionization structure of a gaseous disk rotating around a central Be star in circular, Keplerian orbits is computed, and the profiles of emission lines from the disk studied. Three cases are considered, each modeled on the observations of the shell sta

AB - The ionization structure of a gaseous disk rotating around a central Be star in circular, Keplerian orbits is computed, and the profiles of emission lines from the disk studied. Three cases are considered, each modeled on the observations of the shell sta

M3 - Other contribution

ER -