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Paper: |
Understanding the Structure of the Inner Halo and Bulge |
Volume: |
92, Formation of the Galactic Halo. . . . Inside and Out |
Page: |
92 |
Authors: |
Minniti, Dante |
Abstract: |
Spectroscopic parallaxes for 80 K giants in a bulge field at l, b = (10(deg) , -7.6(deg) ) have been measured. The metal--rich stars have distribution consistent with a barred bulge. The metal--poor stars, on the other hand, are consistent with an axisymmetric system, which is representative of the inner halo. It is argued that bulge and halo are different components. |
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