Spatially resolving the accretion shocks on the rapidly-rotating M0 T-Tauri star MN Lupi
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Strassmeier, K G
Rice, J B
Ritter, A
Kuker, M
Hussain, G
Hubrig, S
Shobbrook, R
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Springer
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We obtained high-resolution, high-quality VLT/UVES spectra to reconstruct the two-dimensional surface structure of the rapidly-rotating classical T-Tauri star MN Lupi on two separate nights. Both surface maps show a structured warm (5000 K) band centered
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Astronomy and Astrophysics
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2037-12-31
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