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Article
New Spectroscopic Technique Based on Coaddition of Surface Brightness Fluctuations: NGC 4449 and Its Stellar Tidal Stream
The Astrophysical Journal (2016)
  • Elisa Toloba, University of California Observatories
  • Puragra Guhathakurta, University of California Observatories
  • Aaron J. Romanowsky, San Jose State University
  • Jean P. Brodie, University of California Observatories
  • David Martínez-Delgado, Universität Heidelberg
  • Jacob A. Arnold, University of California Observatories
  • Neel Ramachandran, St. Francis High School, Mountain View, CA
  • Kuriakose Theakanath, Bellarmine College Preparatory, San Jose, CA
Keywords
  • galaxies: abundances,
  • galaxies: dwarf,
  • galaxies: individual (NGC 4449),
  • galaxies: kinematics and dynamics,
  • galaxies: stellar content
Publication Date
2016
DOI
10.3847/0004-637X/824/1/35
Publisher Statement
This article was originally published in The Astrophysical Journal, volume 824, issue 1. © 2016. The American Astronomical Society. All rights reserved.

This article is also available online at the following link: http://dx.doi.org/10.3847/0004-637X/824/1/35
Citation Information
Elisa Toloba, Puragra Guhathakurta, Aaron J. Romanowsky, Jean P. Brodie, et al.. "New Spectroscopic Technique Based on Coaddition of Surface Brightness Fluctuations: NGC 4449 and Its Stellar Tidal Stream" The Astrophysical Journal Vol. 824 Iss. 1 (2016) ISSN: 0004-637X
Available at: http://works.bepress.com/aaron_romanowsky/108/