NGC 1850 is a bright, double star cluster that lies in the Large Magellanic Cloud, a small neighbor galaxy to the Milky Way. It contains a black hole with a mass of about 11 Suns, and a companion star. No clear detection of X-rays with NASA's Chandra X-ray Observatory implies that the black hole is not quickly pulling material away from its companion. The X-rays are from Chandra (magenta), while the optical are from Hubble Space Telescope (red, yellow, green, cyan, blue) and the infrared from Spitzer Space Telescope (red)
This composite image features a double star cluster, a blue-tinted cloud, and several neon purple dots. This double cluster is part of the Large Magellanic Cloud, a companion galaxy to the Milky Way. The bright, golden stars in the larger cluster fill the upper center of the image. The other cluster is much smaller and coincides with one of the neon purple circles located slightly above and to the right of the image’s center. This and the other purple circles are X-ray sources detected with Chandra. To our left of the combined cluster is a vertical streak of blue-tinted cloud. Extending beyond the upper and lower edges of the image, this section of cloud resembles wafting smoke from a cigarette.
Credit: X-ray: NASA/CXC/SAO; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/J. Major, S. Wolk
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