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A Kiloparsec-Scale Nuclear Stellar Disk in the Milky Way as a Possible Explanation of the High Velocity Peaks in the Galactic Bulge (2015)

First Author: Debattista V

Attributed to: Consolidated Solar and Astrophysics Research at UCLan funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1507.01433

Publication URI: https://arxiv.org/abs/1507.01433

Type: Other