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Modeling Nearly Spherical Pure-bulge Galaxies with a Stellar Mass-to-light Ratio Gradient under the ΛCDM and MOND Paradigms. II. The Orbital Anisotropy of Slow Rotators within the Effective Radius

Crossref DOI link: https://doi.org/10.3847/1538-4357/ab09fd

Published Online: 2019-03-20

Published Print: 2019-03-20

Update policy: https://doi.org/10.1088/crossmark-policy

Authors

Chae, Kyu-Hyun https://orcid.org/0000-0002-6016-2736
Bernardi, Mariangela

Sheth, Ravi K. https://orcid.org/0000-0002-2330-0917
Funding

Funding for this research was provided by:

national research foundation of korea (NRF-2016R1D1A1B03935804)
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Article Title: Modeling Nearly Spherical Pure-bulge Galaxies with a Stellar Mass-to-light Ratio Gradient under the ΛCDM and MOND Paradigms. II. The Orbital Anisotropy of Slow Rotators within the Effective Radius

Journal Title: The Astrophysical Journal

Article Type: paper

Copyright Information: © 2019. The American Astronomical Society. All rights reserved.

Publication dates

Date Received: 2018-10-24

Date Accepted: 2019-02-23

Online publication date: 2019-03-20

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