File:NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars (SVS14434 - transitional pulsar art).webm

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Original file(WebM audio/video file, VP8/Opus, length 21 s, 1,920 × 1,080 pixels, 1.02 Mbps overall, file size: 2.52 MB)

Captions

Captions

This artist's rendering illustrates a possible model for the transitional pulsar J1023. When astronomers can detect pulses in radio (green), the pulsar's energetic outflow holds back its companion's gas stream.

Summary[edit]

Description
English: This artist's rendering illustrates a possible model for the transitional pulsar J1023. When astronomers can detect pulses in radio (green), the pulsar's energetic outflow holds back its companion's gas stream. Sometimes the stream surges, creating a bright disk around the pulsar that can persist for years. The disk shines brightly in X-rays, and gas reaching the neutron star produces jets that emit gamma rays (magenta), obscuring the pulses until the disk eventually dissipates.Credit: NASA's Goddard Space Flight Center
Date 28 November 2023, 14:20:00 (upload date)
Source NASA’s Fermi Mission Finds 300 Gamma-Ray Pulsars
Author NASA's Scientific Visualization Studio - Mark SubbaRao, A. J. Christensen, Francis Reddy, Scott Wiessinger, David A. Smith, Elizabeth Hays
Other versions
Keywords
InfoField
Neutron Star; Space; Ast; Astrophysics; Fermi; 4K; Universe; Pulsar; Milky Way

Licensing[edit]

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current10:35, 15 January 202421 s, 1,920 × 1,080 (2.52 MB)OptimusPrimeBot (talk | contribs)#Spacemedia - Upload of https://svs.gsfc.nasa.gov/vis/a010000/a014400/a014434/transitional_pulsar_art.webm via Commons:Spacemedia

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