Galaxy Rotation Curves Disfavor Traditional and Self-interacting Dark Matter Halos, Preferring a Disk Component or Einasto Function
- Award ID(s):
- 2013199
- NSF-PAR ID:
- 10355191
- Date Published:
- Journal Name:
- The Astrophysical Journal Letters
- Volume:
- 920
- Issue:
- 1
- ISSN:
- 2041-8205
- Page Range / eLocation ID:
- L10
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
More Like this
No document suggestions found
- Free Publicly Accessible Full Text
-
Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.3847/2041-8213/ac1bb7
