Gamma-Ray Eclipsing Binary (IMAGE)

NASA/Goddard Space Flight Center

Gamma-Ray Eclipsing Binary

Caption

An orbiting star begins to eclipse its partner, a rapidly rotating, superdense stellar remnant called a pulsar, in this illustration. The pulsar emits multiwavelength beams of light that rotate in and out of view and produces outflows that heat the star’s facing side, blowing away material and eroding its partner.

Credit

NASA/Sonoma State University, Aurore Simonnet

Usage Restrictions

No restrictions.

License

Public Domain

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