Catalog Service: Young T Tauri star in CB 26 molecular outflows
Description
The disk-outflow connection is thought to play a key role in extracting excess angular momentum from a forming proto-star. Although jet rotation has been observed in a few objects, no rotation of molecular outflows has been unambiguously reported so far. We report new millimeter-interferometric observations of the edge-on T-Tauri-star - disk system in the isolated Bok globule CB-26. The aim of these observations was to study the disk-outflow relation in this 1Myr old low-mass young stellar object.
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This resource was registered on: 2009 Jan 29 00:00:00ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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