The SHARP instrument on the ELT is projected to enable observations of accretion and outflows in very faint young stellar objects down to H~24 mag in the outer Milky Way and Magellanic Clouds using its adaptive optics and multiplexing capabilities.
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SHARPing accretion and outflows in young stellar objects in star forming regions of the outer Galaxy and beyond
The SHARP instrument on the ELT is projected to enable observations of accretion and outflows in very faint young stellar objects down to H~24 mag in the outer Milky Way and Magellanic Clouds using its adaptive optics and multiplexing capabilities.