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<center><H1>Dissertation Abstracts</H1></center>

<H2><A NAME="SECTION00010000000000000000">Beate Woerman</A></H2>
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<B>Radio Observations of the Gum Nebula Region</B><BR> 
<I>Degree and Date: PhD, June 1997<BR> 
Institute: Rhodes University<BR> 
Thesis advisors: Prof. E. Baart, Mr J. Jonas</I><BR>
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ABSTRACT<BR>
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This thesis describes the results of an investigation of the physical
properties of the Gum Nebula. For this investigation a radio continuum map
of the region was made at 2326 MHz and resolution <sup>1</sup>/<sub>3</sub>&#176; with
the Hartebeesthoek Radio Observatory (HartRAO) antenna. This map was used to
generate spectral index images and an infrared to radio flux density ratio
(IRR) image. The latter image shows that the IRR of the nebula is in the
range 20 to 250, identifying it as an old SNR.
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Several spectral index images of this region were generated using two different 
methods, one based on the isolation of the nebula from its background 
radiation, the other based on TT-plots of Turtle <EM>et al.</EM> (MNRAS, 124, 297, 1962). The two methods 
yield similar results, which show that the nebula has a thermal shell with a 
non-thermal region in its interior. Below the galactic plane the thermal 
region dominates and above the plane the nonthermal region. These
results suggest a model of an old SNR with an H&nbsp;II region shell.
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Spectral line observations of hydrogen recombination lines and hydroxyl (OH) 
were made with the HartRAO and the Mopra telescopes.
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The detection of hydrogen recombination lines at four positions in the 
thermal regions of the nebula give electron temperatures and emission measures 
in the ranges 4000 to 6000 K and 220 to 460 pc.cm<sup>-6</sup> respectively. The 
turbulent velocities are of the order of 20 km/s.
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A search for shocked OH lines at 1667 MHz and 1720 MHz in the Gum Nebula gave 
results that were negative, but numerous unshocked 1667 MHz OH lines were detected. The 
latter were used in a test for an expansion of the nebula. The most plausible 
fit to the data gives an expansion centre at <i>l</i> = 260.5&#176;, <i>b</i> = -2.5&#176; and at a distance of 0.7 kpc from us. 
The front face angular radius and expansion velocity are 10.5&#176; and 16 
km/s respectively. The back face angular radius and expansion velocity are 
8.5&#176; and 7 km/s respectively.

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<P><ADDRESS>
<I>Working Group <BR>
Sun Jan 17 10:57:03 GMT+0200 1999</I>
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