The disk-halo interface in edge-on spirals

Details The disk-halo interface in edge-on spirals The disk-halo interface in edge-on spirals

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..326w&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 326-327 (SEE N93-26706 10-90)

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2

Astronomical Spectroscopy, Emission Spectra, H I Regions, Halos, Interstellar Gas, Interstellar Matter, Ionized Gases, Spiral Galaxies, Galactic Nuclei, H Alpha Line, Rosat Mission, Temperature Distribution, X Ray Sources

Scientific paper

We are studying the disk-halo interface in several edge-on spiral galaxies through extensive imagery in H(alpha) and other emission lines from Diffuse Ionized Gas (DIG), also referred to as the Warm Ionized Medium (WIM). In addition, for the nearby Sc galaxy NGC4631 we have obtained x-ray observations with ROSAT, to map the distribution of hot (10(exp 6) - 10(exp 7)) gas in the disk and halo. Here we present initial results for two late-type spirals, NGC4244 and NGC4631.

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