Exif MM * > ; ! Ti v This four-panel graphic shows the two pulsars, Geminga (upper left) and B0355+54 (upper right), observed by Chandra. In both of these images, Chandra's X-rays, colored blue and purple, are combined with infrared data from Spitzer that shows stars in the field of view. Below each data image, an artist's illustration depicts more details of what astronomers think the structure of each pulsar wind nebula looks like. New Chandra data on the shape of these structures may explain the presence or absence of radio and gamma-ray pulses. Chandra X-ray Observatory Center 0221 vhttp://ns.adobe.com/xap/1.0/ This four-panel graphic shows the two pulsars, Geminga (upper left) and B0355+54 (upper right), observed by Chandra. In both of these images, Chandra's X-rays, colored blue and purple, are combined with infrared data from Spitzer that shows stars in the field of view. Below each data image, an artist's illustration depicts more details of what astronomers think the structure of each pulsar wind nebula looks like. New Chandra data on the shape of these structures may explain the presence or absence of radio and gamma-ray pulses. Chandra Images Show That Geometry Solves a Pulsar Puzzle Chandra X-ray Observatory Center Geminga B.3.1.9.1 800 98.4537019 17.7527598 3600.0 3600.0 1801.0 1801.0 2.13637e-05 2.1136736e-05 WCS retrieved using CXCs PinpointWCS adsabs:2016ApJ...833..253K arXiv:1610.06167 arXiv:1611.03496 http://chandra.harvard.edu/photo/image_use.html vPhotoshop 3.0 8BIM 0Z %G 8Chandra Images Show That Geometry Solves a Pulsar Puzzle Geminga7 20170118P Chandra X-ray Observatory Centeri DTwo pulsars about 800 and 3,400 light years from Earth respectively.n X-ray: NASA/CXC/PSU/B.Posselt ets Chandra X-ray ObservatoryxThis four-panel graphic shows the two pulsars, Geminga (upper left) and B0355+54 (upper right), observed by Chandra. In both of these images, Chandra's X-rays, colored blue and purple, are combined with infrared data from Spitzer that shows stars in the field of view. Below each data image, an artist's illustration depicts more details of what astronomers think the structure of each pulsar wind nebula looks like. New Chandra data on the shape of these structures may explain the presence or absence of radio and gamma-ray pulses.8BIM
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