Cosmic Diffuse Far Ultraviolet Emission

Details Cosmic Diffuse Far Ultraviolet Emission Cosmic Diffuse Far Ultraviolet Emission

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.9203e&link_type=abstract

American Astronomical Society, AAS Meeting #211, #92.03; Bulletin of the American Astronomical Society, Vol. 39, p.887

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Scientific paper

Cosmic far-ultraviolet (FUV) spectral-line emission arises from phases of the Galactic interstellar. We have mapped the cosmic FUV line emission over most of the sky. The maps are the final product of the SPEAR mission and include improved data reduction and the isolation and removal of stars. A HEALPIX spectral map in 15 arcminute bins is reduced and presented in distinct spectral lines. Low ionization gas in the cool interstellar media is traced in Si II* and Al II emission, while photo-ionized and thermal gas in the warm to hot interstellar media is traced in C III, C IV, Si IV, O IV], O VI and other emission lines. The FUV sky map data is publicly available.
The SPEAR (FIMS) Mission is supported by NASA grant NAG5-5355 and the Korea Ministry of Science and Technology.

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