Using neutron-capture abundances as a tracer of Galactic halo formation
Fishlock, Cherie; Karakas, Amanda; Lugaro, Maria; Yong, David
Description
Chemical differences in stellar populations are one method to study the formation and evolution of the Galactic halo of the Milky Way. In particular, there are low α-element stars and high α-element stars in the Galactic halo that also show differences
| Collections | ANU Research Publications |
|---|---|
| Date published: | 2013 |
| Type: | Conference paper |
| URI: | http://hdl.handle.net/1885/83054 |
| Source: | Proceedings of Science |
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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Fishlock_Using_neutron-capture_2013.pdf | 532.88 kB | Adobe PDF | Request a copy | |
| 02_Fishlock_Using_neutron-capture_2013.pdf | 87.88 kB | Adobe PDF | Request a copy |
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