Bulge and Nucleus of the Milky Way

The above shows the center of the Milky Way galaxy with the constellation Sagittarius superimposed on the image. The center of the Milky Way sits just above the spout of the teapot. The bulge sits 27,000 light years from the Earth with coordinates RA = 17h45m40.04s and δ = -29:00:28.1 (J2000). The bulge is not easily observed in the visible, UV, or soft x-rays. It is best observed in the γ-ray, hard x-rays, IR, sub-millimeter, and radio.

The bulge of the Milky Way is more spherical than the disk and is composed of stars which are more reddish than those in the disk (===>they are more evolved or low mass, but are still considered Pop I stars). The bulge is roughly 30,000 to 40,000 light years in diameter.

The central region of the Galactic Bulge (the nucleus) is interesting because it shows activity similar to that shown by Active Galactic Nuclei, AGNs (although at a considerably lower level).

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