First stellar abundances in NGC 6822 from VLT-UVES and Keck-Hires spectroscopy

Physics

• Atmospherics 33%
• Be Type Star 33%
• Chemical Evolution 33%
• Data Quality 33%
• Distance 33%
• Dwarf Irregular Galaxies 33%
• Elemental Abundance 33%
• Galaxy Mass 33%
• Gradients 33%
• High Resolution 66%
• Independent Variables 33%
• Iron 100%
• Magellanic Clouds 33%
• Mass 33%
• Metal 33%
• Metallicity 33%
• Model 33%
• Observatories 33%
• Oxygen 100%
• Planetary Atmosphere 33%
• Quality 33%
• Ratios 66%
• Spectra 66%
• Spectrographs 33%
• Spectroscopy 33%
• Stars 66%
• Supergiant 33%
• Underabundance 66%
• Very Large Telescope 66%