Observations of the Diffuse Interstellar Medium in the Far Ultraviolet

Details Observations of the Diffuse Interstellar Medium in the Far Ultraviolet Observations of the Diffuse Interstellar Medium in the Far Ultraviolet

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.9304e&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #93.04D; Bulletin of the American Astronomical Society, Vol. 24, p.1268

Astronomy and Astrophysics

Astrophysics

Scientific paper

Diffuse astrophysical emission at wavelengths between 900 and 1200 Angstroms contains unique information regarding the poorly understood hot phase of the interstellar medium. Limits to diffuse far ultraviolet emission have been obtained with a unique rocket-borne spectrograph. The superior quality of these data provide new constraints to physical properties of the hot interstellar medium. These data, when combined with previous longer wavelength ultraviolet emission observations, also provide bounds to theoretical models of the galactic corona. This work has been supported by NASA contract NGR05-003-450.

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