Bulletin of the American Physical Society
APS April Meeting 2022
Volume 67, Number 6
Saturday–Tuesday, April 9–12, 2022; New York
Session S17: Poster Session III (2:00-4:00 pm)
2:00 PM,
Monday, April 11, 2022
Room: 9th Floor Terrace
Abstract: S17.00065 : Spiral galaxy rotation favors prolate dark matter haloes*
Presenter:
Felipe J Llanes-Estrada
(Univ Complutense)
Authors:
Adriana Bariego Quintana
(Univ. Complutense de Madrid and Univ. Autónoma de Madrid)
Felipe J Llanes-Estrada
(Univ Complutense)
Oliver Manzanilla Carretero
(Univ. Complutense de Madrid)
This theoretical understanding is borne out by the detailed fits to the rotation data that we report: for equal dark matter profile, elongated distributions provide smaller χ^2 than purely spherical ones.
This is of consequence for the estimated dark matter density near Earth.
*Supported by spanish grant MICINN: PID2019-108655GB-I00 (Spain), and Univ. Complutense de Madrid under research group 910309 and the IPARCOS institute.
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700