The authors propose that a long-baseline space interferometer operating in the UV-optical at 0.1 milliarcsecond resolution would enable direct imaging of stellar surfaces, convection, winds, and accretion, transforming stellar astrophysics.
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Stars at High Spatial Resolution
The authors propose that a long-baseline space interferometer operating in the UV-optical at 0.1 milliarcsecond resolution would enable direct imaging of stellar surfaces, convection, winds, and accretion, transforming stellar astrophysics.