Exif II*
\ d ( 1 l 2 ; ! i This enormous W50 cloud, visible only in radio waves, formed when a giant star, 18,000 light years away in the constellation of Aquila, exploded around twenty thousand years ago. The remaining black hole feeds on gas it collects from a very close companion star. Its gas disk and powerful magnetic field lines act like an enormous railroad system. It snags charged particles and channels them outward as powerful jets traveling at nearly the speed of light. This system shines brightly in both radio waves and X-rays and is known collectively as the SS433 microquasar. Over time, the microquasar’s wobbling jets have punched corkscrew bulges on either side of W50, seen here in this image from the Very Large Array (VLA).
- ' - ' Adobe Photoshop CS5.1 Macintosh 2018-01-30T16:39:21-05:00 NRAO/AUI/NSF https://public.nrao.edu/mediause 0220 [ [ 5http://ns.adobe.com/xap/1.0/ 18E+03 0.00000000000000 -1.17656704245946 1.26807973749272e-03 0.00000000000000 5.00000000000000 ArcSinh(x) 8.38713090512354 VLA VLA WISE WISE WISE World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center 23001371 2409.17510275476 1453.16023174640 287.95416666667 4.98666666667 -0.00083073762 0.00083073762 Radio Radio Infrared Infrared Infrared L L I I I 1.835E+08 1.835E+08 3.4E+03 12E+03 4.6E+03 Cyan Cyan Blue Red Green C.4.1.4 2011-01-15T13:13:28.250001 2011-01-15T13:13:28.250001 Wed Mar 07 16:08:25 EST 2012 Wed Mar 07 16:16:27 EST 2012 Wed Mar 07 16:12:28 EST 2012 NRAO/AUI/NSF This enormous W50 cloud, visible only in radio waves, formed when a giant star, 18,000 light years away in the constellation of Aquila, exploded around twenty thousand years ago. The remaining black hole feeds on gas it collects from a very close companion star. Its gas disk and powerful magnetic field lines act like an enormous railroad system. It snags charged particles and channels them outward as powerful jets traveling at nearly the speed of light. This system shines brightly in both radio waves and X-rays and is known collectively as the SS433 microquasar. Over time, the microquasar’s wobbling jets have punched corkscrew bulges on either side of W50, seen here in this image from the Very Large Array (VLA).
https://public.nrao.edu/mediause W50 SS433 Microquasar W50: The Manatee Nebula xmp.did:04801174072068119109B887DC4441A0 Creative Commons Attribution 3.0 Unported license (http://creativecommons.org/licenses/by/3.0/) https://public.nrao.edu/gallery/w50-the-manatee-nebula/ 5http://ns.adobe.com/xap/1.0/ 18E+03 0.00000000000000 -1.17656704245946 1.26807973749272e-03 0.00000000000000 5.00000000000000 ArcSinh(x) 8.38713090512354 VLA VLA WISE WISE WISE World Coordinate System resolved using PinpointWCS 0.9.2 revision 218+ by the Chandra X-ray Center 23001371 2409.17510275476 1453.16023174640 287.95416666667 4.98666666667 -0.00083073762 0.00083073762 Radio Radio Infrared Infrared Infrared L L I I I 1.835E+08 1.835E+08 3.4E+03 12E+03 4.6E+03 Cyan Cyan Blue Red Green C.4.1.4 2011-01-15T13:13:28.250001 2011-01-15T13:13:28.250001 Wed Mar 07 16:08:25 EST 2012 Wed Mar 07 16:16:27 EST 2012 Wed Mar 07 16:12:28 EST 2012 NRAO/AUI/NSF This enormous W50 cloud, visible only in radio waves, formed when a giant star, 18,000 light years away in the constellation of Aquila, exploded around twenty thousand years ago. The remaining black hole feeds on gas it collects from a very close companion star. Its gas disk and powerful magnetic field lines act like an enormous railroad system. It snags charged particles and channels them outward as powerful jets traveling at nearly the speed of light. This system shines brightly in both radio waves and X-rays and is known collectively as the SS433 microquasar. Over time, the microquasar’s wobbling jets have punched corkscrew bulges on either side of W50, seen here in this image from the Very Large Array (VLA).
https://public.nrao.edu/mediause W50 SS433 Microquasar W50: The Manatee Nebula xmp.did:04801174072068119109B887DC4441A0 Creative Commons Attribution 3.0 Unported license (http://creativecommons.org/licenses/by/3.0/) https://public.nrao.edu/gallery/w50-the-manatee-nebula/ Photoshop 3.0 8BIM Z %G xThis enormous W50 cloud, visible only in radio waves, formed when a giant star, 18,000 light years away in the constellation of Aquila, exploded around twenty thousand years ago. The remaining black hole feeds on gas it collects from a very close companion star. Its gas disk and powerful magnetic field lines act like an enormous railroad system. It snags charged particles and channels them outward as powerful jets traveling at nearly the speed of light. This system shines brightly in both radio waves and X-rays and is known collectively as the SS433 microquasar. Over time, the microquasar’s wobbling jets have punched corkscrew bulges on either side of W50, seen here in this image from the Very Large Array (VLA).
i W50: The Manatee Nebula
P NRAO/AUI/NSFn B. Saxton, (NRAO/AUI/NSF) from ds NRAO/AUI/NSF W50: The Manatee Nebula W50 SS433 Microquasart https://public.nrao.edu/mediause8BIM% e4R5ۦ Adobe d
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