Mapping the Galactic Halo. V. Sagittarius Dwarf Spheroidal Tidal Debris 60� from the Main Body
As part of the Spaghetti Project Survey, we have detected a concentration of giant stars well above expectations for a smooth halo model. The position (l ∼ 350°, b ∼ 50°) and distance (∼50 kpc) of this concentration match those of the northern ove
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
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