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A New Class Of X-ray Star?

A New Class Of X-ray Star?


Depicts: Illustration of gamma Cassiopeia's B-emission
Copyright: M. Smith (ST ScI) and NASA

The team pointed both the Hubble Space Telescope and the Rossi X-Ray Timing Explorer at the hot star gamma Cassiopeiae, simultaneously for one full day in March, 1996 in order to understand the origin of the bright, variable X-rays coming from this star. To their surprise they discovered the X-rays are probably produced by extraordinarily hot surface flares, which are completely unexpected and unpredicted for a star of this type.
Last Update: 1 September 2019
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25-Apr-2024 17:43 UT

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