Английская Википедия:DG Tauri B

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Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox astrometry Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end

DG Tauri B, near the T Tauri star DG Tauri,[1] is a young stellar object located 450 light-years (140 parsecs) from Earth, within the Taurus constellation.[2] Observations of DG Tauri B were first made in October, and later December 1995 at the 6 element Owens Valley millimeter wave array.[3] Its most notable characteristics are its bipolar jets of molecular gas and dust emanating from either side of the object.[2][3] Red-shifted carbon monoxide emissions extend out 6,000 AU to the northwest of the object from the undetermined source, and are symmetrically distributed about the jet, while blue-shifted CO emissions are confined to a region with a roughly 500 AU radius.[3]

References

Шаблон:Reflist

Шаблон:Stars of Taurus


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