The 3D structure of the galactic bulge from the MACHO red clump stars

Details The 3D structure of the galactic bulge from the MACHO red clump stars The 3D structure of the galactic bulge from the MACHO red clump stars

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001iaus..205..234f&link_type=abstract

Galaxies and their Constituents at the Highest Angular Resolutions, Proceedings of IAU Symposium #205, held 15-18 August 2000 at

Physics

Scientific paper

The MACHO experiment has surveyed some 2 million red clump stars in a roughly 8o× 8o area of the Galactic bulge centred on (l,b)=(4o,-6o). These stars have reliable photometric distances and are used as tracer for a preliminary derivation of the three-dimensional structure of the Milky Way's bulge/bar.

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