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Updated: Mar 7, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
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An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907

Gian Luca Israel1, Andrea Belfiore2, Luigi Stella3

  • 1Osservatorio Astronomico di Roma, Istituto Nazionale di Astrofisica (INAF), via Frascati 33, I-00078 Monteporzio Catone, Italy. gianluca@oa-roma.inaf.it.

Science (New York, N.Y.)
|February 22, 2017
PubMed

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