New Spectroscopic Technique Based on Coaddition of Surface Brightness Fluctuations: NGC 4449 and Its Stellar Tidal Stream

Authors

Elisa Toloba, University of California Observatories
Puragra Guhathakurta, University of California Observatories
Aaron Romanowsky, San Jose State UniversityFollow
Jean Brodie, University of California Observatories
David Martínez-Delgado, Universität Heidelberg
Jacob Arnold, University of California Observatories
Neel Ramachandran, St. Francis High School, Mountain View, CA
Kuriakose Theakanath, Bellarmine College Preparatory, San Jose, CA

Document Type

Article

Publication Date

January 2016

Publication Title

The Astrophysical Journal

Volume

824

Issue Number

1

DOI

10.3847/0004-637X/824/1/35

Keywords

galaxies: abundances, galaxies: dwarf, galaxies: individual (NGC 4449), galaxies: kinematics and dynamics, galaxies: stellar content

Disciplines

Astrophysics and Astronomy | External Galaxies

Comments

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

Recommended Citation

Elisa Toloba, Puragra Guhathakurta, Aaron Romanowsky, Jean Brodie, David Martínez-Delgado, Jacob Arnold, Neel Ramachandran, and Kuriakose Theakanath. "New Spectroscopic Technique Based on Coaddition of Surface Brightness Fluctuations: NGC 4449 and Its Stellar Tidal Stream" The Astrophysical Journal (2016). https://doi.org/10.3847/0004-637X/824/1/35