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A Tale of Two Type Ia Supernovae: The Fast-declining Siblings SNe 2015bo and 1997cn
W. B. Hoogendam, C. Ashall, L. Galbany, B. J. Shappee, C. R. Burns, J. Lu, M. M. Phillips, E. Baron, S. Holmbo, E. Y. Hsiao, N. Morrell, M. D. Stritzinger, N. B. Suntzeff, F. Taddia, D. R. Young, J. D. Lyman, S. Benetti, P. A. Mazzali, M. Delgado Mancheño, R. González Díaz and S. Muñoz Torres The Astrophysical Journal 928(2) 103 (2022) https://doi.org/10.3847/1538-4357/ac54aa
The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The kinematic diversity of stellar halos and the relation between halo transition scale and stellar mass
Dwarf galaxy populations in present-day galaxy clusters - I. Abundances and red fractions
Simone M. Weinmann, Thorsten Lisker, Qi Guo, Hagen T. Meyer and Joachim Janz Monthly Notices of the Royal Astronomical Society 416(2) 1197 (2011) https://doi.org/10.1111/j.1365-2966.2011.19118.x
Gravitational stability and dynamical overheating of galactic stellar disks
DISSIPATION AND EXTRA LIGHT IN GALACTIC NUCLEI. III. “CORE” ELLIPTICALS AND “MISSING” LIGHT
Philip F. Hopkins, Tod R. Lauer, Thomas J. Cox, Lars Hernquist and John Kormendy The Astrophysical Journal Supplement Series 181(2) 486 (2009) https://doi.org/10.1088/0067-0049/181/2/486
STRUCTURE AND FORMATION OF ELLIPTICAL AND SPHEROIDAL GALAXIES
The Evolution of Early‐Type Galaxies in Distant Clusters. II. Internal Kinematics of 55 Galaxies in the \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 $z=0.33$ \end{document} Cluster Cl 1358+62
Daniel D. Kelson, Garth D. Illingworth, Pieter G. van Dokkum and Marijn Franx The Astrophysical Journal 531(1) 159 (2000) https://doi.org/10.1086/308445