Edward A Ajhar
Affiliations: | National Science Foundation, Arlington, VA, United States |
Area:
cosmology; extragalactic astronomyGoogle:
"Edward Ajhar"Mean distance: (not calculated yet)
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Publications
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Ferrarese L, Mould JR, Stetson PB, et al. (2007) The discovery of cepheids and a distance to NGC 5128 Astrophysical Journal. 654: 186-218 |
Lauer TR, Faber SM, Gebhardt K, et al. (2005) The centers of early-type galaxies with Hubble Space Telescope. V. New WFPC2 photometry Astronomical Journal. 129: 2138-2185 |
Jensen JB, Tonry JL, Barris BJ, et al. (2003) Measuring distances and probing the unresolved stellar populations of galaxies using infrared surface brightness fluctuations Astrophysical Journal. 583: 712-726 |
Ajhar EA, Tonry JL, Blakeslee JP, et al. (2001) Reconciliation of the surface brightness fluctuation and type Ia supernova distance scales Astrophysical Journal. 559: 584-591 |
Jensen JB, Tonry JL, Thompson RI, et al. (2001) The Infrared Surface Brightness Fluctuation Hubble Constant The Astrophysical Journal. 550: 503-521 |
Tontry JL, Dressler A, Blakeslee JP, et al. (2001) The SBF survey of galaxy distances. IV. SBF magnitudes, colors, and distances Astrophysical Journal. 546: 681-693 |
Blakeslee JP, Vazdekis A, Ajhar EA. (2001) Stellar populations and surface brightness fluctuations: new observations and models Monthly Notices of the Royal Astronomical Society. 320: 193-216 |
Tonry JL, Blakeslee JP, Ajhar EA, et al. (2000) The Surface Brightness Fluctuation Survey of Galaxy Distances. II. Local and Large-Scale Flows* ** The Astrophysical Journal. 530: 625-651 |
Kelson DD, Illingworth GD, Tonry JL, et al. (2000) 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 The Astrophysical Journal. 529: 768-785 |
Gebhardt K, Richstone D, Kormendy J, et al. (2000) Axisymmetric, three-integral models of galaxies: A massive black hole in NGC 3379 Astronomical Journal. 119: 1157-1171 |