Argos - III. Stellar populations in the galactic bulge of the milky way
We present the metallicity results from the ARGOS spectroscopic survey of the Galactic bulge. Our aim is to understand the formation of the Galactic bulge: did it form via mergers, as expected from Λ cold dark matter theory, or from disc instabilities, a
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Ness_Argos_-_III._Stellar_2013.pdf||3.7 MB||Adobe PDF|
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