Using
Many barred galaxies exhibit upturns (shoulders) in their bar-major-axis density profile. Simulation studies have suggested that shoulders are supported by looped
- Award ID(s):
- 2009122
- NSF-PAR ID:
- 10462855
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 955
- Issue:
- 1
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 38
- Size(s):
- ["Article No. 38"]
- Sponsoring Org:
- National Science Foundation
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