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      TheHubble Space TelescopeKey Project on the Extragalactic Distance Scale. XXVII. A Derivation of the Hubble Constant Using the Fundamental Plane and \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} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $D_{n}$ \end{document} ‐σ Relations in Leo I, Virgo, and Fornax

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          Precision photometry of early-type galaxies in the Coma and Virgo clusters: a test of the universality of the colour-magnitude relation - II. Analysis

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            A Precise Distance Indicator: Type Ia Supernova Multicolor Light‐Curve Shapes

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              On the shape of the light profiles of early-type galaxies

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                Author and article information

                Journal
                The Astrophysical Journal
                ApJ
                University of Chicago Press
                0004-637X
                1538-4357
                February 2000
                February 2000
                : 529
                : 2
                : 768-785
                Article
                10.1086/308310
                39f19af7-f173-4130-a344-afd555a9de43
                © 2000
                History

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