Chandra's image of the Galactic Center (left) has provided evidence for a new and unexpected way for stars to form. A combination of infrared and X-ray observations indicates that a surplus of massive stars has formed from a large disk of gas around Sagittarius A*, the Milky Way's central black hole (illustration on right). Credit: X-ray: NASA/CXC/MIT/F.K.Baganoff et al.; Illustration: NASA/CXC/M.Weiss
The above story is based on materials provided by Chandra X-ray Center. Note: Materials may be edited for content and length.
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Chandra X-ray Center. "NASA's Chandra Reveals New Star Generation." ScienceDaily. ScienceDaily, 14 October 2005. <www.sciencedaily.com/releases/2005/10/051014072125.htm>.
Chandra X-ray Center. (2005, October 14). NASA's Chandra Reveals New Star Generation. ScienceDaily. Retrieved March 7, 2014 from www.sciencedaily.com/releases/2005/10/051014072125.htm
Chandra X-ray Center. "NASA's Chandra Reveals New Star Generation." ScienceDaily. www.sciencedaily.com/releases/2005/10/051014072125.htm (accessed March 7, 2014).