Galactic Center
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Type of Object: The center of the Milky Galaxy probably contains a supermassive (several million times the mass of our sun) black hole. The galactic center is called SGR-A*. The area surrounding SGR-A* contains emission of light from across the electromagnetic spectrum. The center is obscured by dust clouds in the interstellar medium - so most of our observations are made in the near-infrared and radio parts of the spectrum. Distance: 26,000 light years Other Names: Galactic Center, W 24 Radio Brightness at 1420 MHz (21 cm): 2000 Jy Some Links |
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Imagesshown below, at different wavelengths, cover a |

Visible image from the digitized Palomar Sky Survey E plates. The galactic center is obscured in the visible by interstellar clouds. Some faint emission can be seen.

Far-Infrared falso-color image at 100 microns taken by the Infrared Astronomical Satellite (IRAS) Survey. Shows warm dust along the galactic center.

False-color image taken at the radio emission of neutral hydrogen at 1420 MHz by the NRAO VLA Sky Survey. Shows gas component of the galactic center.

False-color image taken at the radio emission frequency of 4850 MHz. Image shows the gas component.. Image is from a Green Bank survey from 0° to +75° declination).
