Image Details
Caption: Fig. 3.
Surface shape (top two panels) and temperature profile (bottom panel) showing the disk source models used for outbursting (solid lines) and quiescent (dashed lines) simulations. All three panels have the same radial scale expressed in either ﹩R_{\odot }﹩ or AU. The top panel shows the disk’s true proportions.
© 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.