Pulsars Emit Gamma-rays from Equator
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- Visualizations by:
- Cruz deWilde
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A pulsar is a rapidly spinning and highly magnetized neutron star, the crushed core left behind when a massive sun explodes. Most were found through their pulses at radio wavelengths, which are thought to be caused by narrow, lighthouse-like beams emanating from the star's magnetic poles.
When it comes to gamma-rays, pulsars are no longer lighthouses. A new class of gamma-ray-only pulsars shows that the gamma rays must form in a broader region than the lighthouse-like radio beam. Astronomers now believe the pulsed gamma rays arise far above the neutron star.
Credits
Please give credit for this item to:
NASA/Fermi/Cruz deWilde
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Animator
- Cruz deWilde (Avant Gravity) [Lead]
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Scientist
- Steven Ritz (NASA/GSFC)
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Producer
- Stefanie Misztal (UMBC)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
Fermi (Collected with the LAT sensor)
Event List
Fermi Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT)
Dataset can be found at: http://fermi.gsfc.nasa.gov
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details, nor the data sets themselves on our site.
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