Nitrogen V in the Wind of the Pre-Main Sequence Herbig Ae Star AB Aur
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Recent GHRS observations of the Herbig Ae star AB Aur demonstrate the presence of N V in the wind of this star. We found that models including hot (T≈140,000 K) clumps are able to reproduce the available observations and are also consistent with its X-ray emission.
KeywordsFilling Factor High Temperature Zone Alfven Wave Corotating Interaction Region Energy Radiative Loss
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