Understanding the Structure of the Inner Halo and Bulge

Details Understanding the Structure of the Inner Halo and Bulge Understanding the Structure of the Inner Halo and Bulge

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aspc...92...92m&link_type=abstract

Formation of the Galactic Halo...Inside and Out, ASP Conference Series, Vol. 92, 1996, Heather Morrison and Ata Sarajedini, eds.

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Scientific paper

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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