Interstellar, intracluster and supercluster gas

Details Interstellar, intracluster and supercluster gas Interstellar, intracluster and supercluster gas

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981xras.nasa..119c&link_type=abstract

In NASA. Goddard Space Flight Center X-ray Astronomy in the 1980's p 119-132 (SEE N82-26055 16-88)

Astronomy and Astrophysics

Astronomy

Dense Plasmas, High Temperature Plasmas, Interstellar Gas, Spectral Resolution, Spectrum Analysis, Angular Resolution, Bremsstrahlung, High Resolution, Stellar Winds, X Ray Astronomy

Scientific paper

Hot tenuous plasmas with temperatures in the range 1,000,000 to 3.10 to the 8th power K and densities of .000001 to .001 per cu cm are considered. The dominant radiation processes are thermal bremsstrahlung and collisional line excitation and all except the very hottest objects will have observable X-ray emissions lines. The most important unifying point is the angular scales involved. For the interstellar gas, structure ranging in size from about 10 ft to tens of degrees is expected.

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