"Small Scatter and Nearly Isothermal Mass Profiles to Four Half-Light Radii from Two-Dimensional Stellar Dynamics of Early-Type Galaxies" by Michele Cappellari

Article

Small Scatter and Nearly Isothermal Mass Profiles to Four Half-Light Radii from Two-Dimensional Stellar Dynamics of Early-Type Galaxies

The Astrophysical Journal Letters (2015)

Michele Cappellari, University of Oxford
Aaron J. Romanowsky, San Jose State University
Jean P. Brodie, University of California Observatories
Duncan A. Forbes, Swinburne University of Technology
Jay Strader, Michigan State University
Caroline Foster, Australian Astronomical Observatory
Sreeja S. Kartha, Swinburne University of Technology
Nicola Pastorello, Swinburne University of Technology
Vincenzo Pota, Swinburne University of Technology
Lee R. Spitler, Australian Astronomical Observatory
Christopher Usher, Swinburne University of Technology
Jacob A. Arnold, University of California Observatories

Download Find in your library

Keywords

galaxies: elliptical and lenticular cD,
galaxies: formation,
galaxies: kinematics and dynamics,
galaxies: structure

Disciplines

Publication Date

2015

DOI

10.1088/2041-8205/804/1/L21

Publisher Statement

Originally published in The Astrophysical Journal Letters, volume 804, issue 1, article 21, 2015. Available online at: http://dx.doi.org/10.1088/2041-8205/804/1/L21

Citation Information

Michele Cappellari, Aaron J. Romanowsky, Jean P. Brodie, Duncan A. Forbes, et al.. "Small Scatter and Nearly Isothermal Mass Profiles to Four Half-Light Radii from Two-Dimensional Stellar Dynamics of Early-Type Galaxies" The Astrophysical Journal Letters Vol. 804 Iss. 1 (2015) ISSN: 2041-8205
Available at: http://works.bepress.com/aaron_romanowsky/110/