Outer Spiral Disks as Clues to Galaxy Formation and Evolution
arXiv:1003.2565 · doi:10.1071/AS09067
Abstract
Recent studies of outer spiral disks have given rise to an abundance of new results. We discuss the observational and theoretical advances that have spurred the interest in disk outskirts, as well as where we currently stand in terms of our understanding of outer disk structure, ages and metallicities.
5 pages, 2 figures. Accepted for publication in PASA. Invited review given at Galaxy Metabolism: Galaxy Evolution near and far, Sydney, 22-26 June 2009.
References in corpus (9)
- Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
- Color Profiles of Spiral Galaxies: Clues on Outer-Disk Formation Scenarios
- Antitruncated Stellar Disks via Minor Mergers
- On the formation of extended galactic disks by tidally disrupted dwarf galaxies
- Stellar populations across the NGC4244 truncated galactic disk
- The Abundance Gradient in the Extremely Faint Outer Disk of NGC 300
- Disk galaxies with broken luminosity profiles from cosmological simulations
- The Stellar Populations of M33's Outer Regions II: Deep ACS Imaging
- The Disk and Extraplanar Environment of NGC 247
Cited by in corpus (4)
- The age structure of stellar populations in the solar vicinity. Clues of a two-phase formation history of the Milky Way disk
- Radial distribution of gas and dust in the two spiral galaxies M99 and M100
- In search of cool flow accretion onto galaxies where does the disk gas end?
- Outside-in stellar formation in the spiral galaxy M33?