Non equilibrium ionization in the local hot bubble

Details Non equilibrium ionization in the local hot bubble Non equilibrium ionization in the local hot bubble

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2345..301a&link_type=abstract

In NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81 p 301-304 (SEE N85-15539 06-90)

Astronomy and Astrophysics

Astronomy

5

Bubbles, Celestial Sphere, Emissivity, Interstellar Matter, Nonequilibrium Ionization, Softening, Supernova Remnants, X Ray Spectroscopy, Astronomical Models, Celestial Bodies, Ion Exchanging, Solar System, Spaceborne Astronomy

Scientific paper

Soft X-ray surveys proved the existence of a local hot bubble surrounding the solar system (McCammon et al. 1983). Recently two experiments measured the spectrum of this hot interstellar medium with solid state detectors during rocket flights between 300 and 1000 eV (Rocchia et al. 1984). The good resolution of the experiment permitted to measure C V, C VI and O VII line emissivities with good accuracy. The authors use these data to put some constraints on a model where the emission comes from a supernova remnant expanding in a finite pressure medium (Cox and Anderson 1982). They show the importance of non equilibrium ionization phenomena.

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