Radio astronomy techniques : the use of radio instruments from single dish radio telescopes to radio interferometers
New radio telescopes under development, will significantly enhance the capabilities of radio astronomy in the Southern Hemisphere. South Africa, in particular, is actively involved in the development of a new array (MeerKAT) as well as in the expansion of existing very long baseline interferomete...
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| Language: | en |
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2012
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| Online Access: | De Witt, Aletha (2012) Radio astronomy techniques : the use of radio instruments from single dish radio telescopes to radio interferometers, University of South Africa, Pretoria, <http://hdl.handle.net/10500/7046> http://hdl.handle.net/10500/7046 |
| Summary: | New radio telescopes under development, will significantly enhance the capabilities
of radio astronomy in the Southern Hemisphere. South Africa, in
particular, is actively involved in the development of a new array (MeerKAT)
as well as in the expansion of existing very long baseline interferometer arrays
in the south. Participation in these new developments demands a thorough
understanding of radio astronomy techniques, and data analysis, and this
thesis focusses on two projects with the aim of gaining such experience.
The Southern Hemisphere very long baselines array is not well served
with calibrator sources and there are significant gaps in the present calibrator
distribution on the sky. An adequately dense, well distributed, set of strong,
compact calibrator or reference sources is needed. With this in mind, observations
using the Southern Hemisphere long baseline array were conducted to
investigate a sample of candidate calibrator sources. The compactness of the
sources was investigated and new potential calibrators have been identified.
Single antenna radio spectroscopy of OH masers has identified sources
of 1720 MHz emission associated with supernova remnants at the shock interface
between the expanding supernova remnant and a molecular cloud.
Models indicate that these masers are shock excited and can only be produced
under tight physical constraints. Out
ows from newly-formed stars
create nebulous regions known as Herbig-Haro objects when they interact
with the surrounding medium, and these regions are potentially similar to
those seen in supernova remnants. If conditions behind the shock fronts of
Herbig-Haro objects are able to support 1720-MHz OH masers they could
be a useful diagnostic tool for star formation. A survey toward Herbig-Haro
objects using a single-dish radio telescope did detect 1720-MHz OH lines in
emission, but neither their spectral signature nor follow-up observations with
the Very Large Array showed evidence of maser emission. === Mathematical Sciences === Ph.D. (Astronomy) |
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