SPEAR far UV spectral imaging of highly ionized emission from the North Galactic Pole Region

Details SPEAR far UV spectral imaging of highly ionized emission from the North Galactic Pole Region SPEAR far UV spectral imaging of highly ionized emission from the North Galactic Pole Region

2007-06-06

arxiv.org/abs/0706.0927v1

Astronomy and Astrophysics

Astrophysics

5 figures

Scientific paper

10.1051/0004-6361:20077685

We present far ultraviolet (FUV: 912 - 1750AA) spectral imaging observations recorded with the SPEAR satellite of the interstellar OVI (1032AA), CIV (1550AA), SiIV (1394AA), SiII* (1533AA) and AlII (1671AA) emission lines originating in a 60 x 30 degree rectangular region lying close to the North Galactic Pole. These data represent the first large area, moderate spatial resolution maps of the distribution of UV spectral-line emission originating the both the highly ionized medium (HIM) and the warm ionized medium (WIM) recorded at high galactic latitudes.

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