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- W2022296068 abstract "ABSTRACT We examine a simple model to account for the observations during quiescence of the soft X‐ray transients within the context of the standard accretion disk limit cycle. In our model the cooling front is not able to propagate completely to the inner edge of the accretion disk, so that a portion of the inner disk is always in the high state. The outer edge documentclass{aastex} usepackage{amsbsy} usepackage{amsfonts} usepackage{amssymb} usepackage{bm} usepackage{mathrsfs} usepackage{pifont} usepackage{stmaryrd} usepackage{textcomp} usepackage{portland,xspace} usepackage{amsmath,amsxtra} usepackage[OT2,OT1]{fontenc} newcommandcyr{ renewcommandrmdefault{wncyr} renewcommandsfdefault{wncyss} renewcommandencodingdefault{OT2} normalfont selectfont} DeclareTextFontCommand{textcyr}{cyr} pagestyle{empty} DeclareMathSizes{10}{9}{7}{6} begin{document} landscape $r_{mathrm{crit},}$ end{document} of this hot, ionized disk determines the rate of accretion and maximum temperature in..." @default.
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- W2022296068 date "2000-10-01" @default.
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- W2022296068 title "A Hot Inner Disk during the Quiescent State of Soft X‐Ray Transients?" @default.
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