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Current Radio Current Radio Sources Sources Crystal Rattazzi, Crystal Rattazzi, Becky Harris, Shawn Becky Harris, Shawn Peters, Chuck Fultz, Peters, Chuck Fultz, Matt Storey, Zach Matt Storey, Zach Brown Brown

Current Radio Sources

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Current Radio Sources. Crystal Rattazzi, Becky Harris, Shawn Peters, Chuck Fultz, Matt Storey, Zach Brown. Cygnus A Extra Galactic Source. Sagittarius A Galactic Center. Jupiter Planetary Radio Source. Crab Nebula Supernova Remnant. 2237+0305 Quasar. SS433 Binary Star System. - PowerPoint PPT Presentation

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Page 1: Current Radio Sources

Current Radio SourcesCurrent Radio Sources

Crystal Rattazzi, Becky Harris, Crystal Rattazzi, Becky Harris, Shawn Peters, Chuck Fultz, Shawn Peters, Chuck Fultz,

Matt Storey, Zach BrownMatt Storey, Zach Brown

Page 2: Current Radio Sources

Cygnus A Cygnus A Extra Galactic SourceExtra Galactic Source

Page 3: Current Radio Sources

Sagittarius ASagittarius AGalactic CenterGalactic Center

Page 4: Current Radio Sources

JupiterJupiterPlanetary Radio SourcePlanetary Radio Source

Page 5: Current Radio Sources

Crab NebulaCrab NebulaSupernova Remnant Supernova Remnant

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2237+03052237+0305QuasarQuasar

Page 7: Current Radio Sources

SS433SS433Binary Star SystemBinary Star System

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Pulsar SourcesPulsar SourcesPSR B0329+54PSR B0329+54

This pulsar is a typical, normal pulsar, rotating with a period of 0.714519 This pulsar is a typical, normal pulsar, rotating with a period of 0.714519 seconds, i.e. close to 1.40 rotations/sec.seconds, i.e. close to 1.40 rotations/sec.

http://www.jb.man.ac.uk/~pulsar/Education/Sounds/B0329.auhttp://www.jb.man.ac.uk/~pulsar/Education/Sounds/B0329.au

PSR B0833-45, The Vela PulsarPSR B0833-45, The Vela PulsarThis pulsar lies near the centre of the Vela supernova remnant, which is the This pulsar lies near the centre of the Vela supernova remnant, which is the debris of the explosion of a massive star about 10,000 years ago. The pulsar debris of the explosion of a massive star about 10,000 years ago. The pulsar is the collapsed core of this star, rotating with a period of 89 milliseconds or is the collapsed core of this star, rotating with a period of 89 milliseconds or about 11 times a second.about 11 times a second.

http://www.jb.man.ac.uk/~pulsar/Education/Sounds/vela.auhttp://www.jb.man.ac.uk/~pulsar/Education/Sounds/vela.au

PSR B0531+21, The Crab PulsarPSR B0531+21, The Crab PulsarThis is the youngest known pulsar and lies at the centre of the Crab Nebula, This is the youngest known pulsar and lies at the centre of the Crab Nebula, the supernova remnant of its birth explosion, which was witnessed by the supernova remnant of its birth explosion, which was witnessed by Europeans and Chinese in the year 1054 A.D. as a day-time light in the sky. Europeans and Chinese in the year 1054 A.D. as a day-time light in the sky. The pulsar rotates about 30 times a second.The pulsar rotates about 30 times a second.

http://www.jb.man.ac.uk/~pulsar/Education/Sounds/crab.auhttp://www.jb.man.ac.uk/~pulsar/Education/Sounds/crab.au

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Phase I - Cylinder Template Phase I - Cylinder Template