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Pulsar-based map of galactic acceleration

Published:2024-06-10 Issue:12 Volume:109 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Moran Abigail¹²^ORCID,Mingarelli Chiara M. F.³²⁴^ORCID,Van Tilburg Ken⁴⁵^ORCID,Good Deborah⁶²⁴

Affiliation:

1. Columbia University

2. University of Connecticut

3. Yale University

4. Flatiron Institute

5. New York University

6. University of Montana

Funder

Simons Foundation

National Science Foundation

National Aeronautics and Space Administration

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.109.123015/fulltext

Reference74 articles.

1. The Circular Velocity Curve of the Milky Way from 5 to 25 kpc

2. Uncertainties in the Galactic Dark Matter distribution: An update

3. A Milky Way with a massive, centrally concentrated thick disc: new Galactic mass models for orbit computations

4. The mass distribution in the galactic disc - II. Determination of the surface mass density of the galactic disc near the Sun

5. The local density of matter mapped by Hipparcos

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Galactic structure from binary pulsar accelerations: Beyond smooth models;Physical Review D;2024-07-18

2. Pulsar-based map of galactic acceleration;Physical Review D;2024-06-10

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