Galactic Oxygen-Rich Supernova Remnant
G292.0+1.8
Left:True-color image of G292.0+1.8 from the Chandra/ACIS observation. Red, green, and blue represent 0.3-0.8 keV, 0.85-1.7 keV, and 1.7-8.0 keV, respectively. Right: The 2-7 keV band image showing the central hard point source - the pulsar (PSR J1124-5916; Camilo et al. 2002, ApJ, 567L, 71C) and its wind nebula.

Hughes et al. 2001, ApJ, 559, L153
Park et al. 2002, ApJ, 564, L39
Hughes et al. 2003, ApJ, 591, L139
Park et al. 2004, ApJ, 602, L33

Back to the Penn State SNR home page

Last update of web pages on SNR 1987A, August 12, 2002, by Sangwook Park (park@astro.psu.edu)

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Pen n State's High Energy Astrophysics group web pages are maintained by Scott Koch.

Last update:  December 16, 1997