Concepts for a high-resolution multi-object spectrograph for galactic archeology on the Anglo-Australian Telescope
Mapping out stellar families to trace the evolutionary star formation history of the Milky Way requires a spectroscopic facility able to deliver high spectral resolution (R 30k) with both good wavelength coverage (~400 Ang) and target multiplex advantage
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|Source:||Ground-Based and Airborne Instrumentation for Astronomy II|
|01_Barden_Concepts_for_a_high-resolution_2008.pdf||860.9 kB||Adobe PDF||Request a copy|
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