Laboratory Astrophysics Survey Of Key X-Ray Diagnostic Lines Using A Microcalorimeter On An Electron Beam Ion Trap

Details Laboratory Astrophysics Survey Of Key X-Ray Diagnostic Lines Using A Microcalorimeter On An Electron Beam Ion Trap Laboratory Astrophysics Survey Of Key X-Ray Diagnostic Lines Using A Microcalorimeter On An Electron Beam Ion Trap

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..dmp..j602s&link_type=abstract

American Physical Society, DAMOP Meeting, 14-June 17, 2000 Storrs, CT, abstract #J6.02

Astronomy and Astrophysics

Astrophysics

Scientific paper

Cosmic plasma conditions created in an Electron Beam Ion Trap (EBIT) make it possible to simulate the dependencies of key diagnostic x-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources. We used a microcalorimeter coupled with an x-ray optic to measure broad band spectra obtained from the NIST EBIT with an energy resolution approaching that of a Bragg crystal spectrometer. Spectra are presented for nitrogen, oxygen, neon, argon , and iron in various stages of ionization.

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