Results
author = "Green, A.J."
Opportunities for maser studies with the Square Kilometre Array
Description :
The Square Kilometre Array (SKA) is the radio telescope of the next
generation, providing an increase in sensitivity and angular resolution of two
orders of magnitude over existing telescopes. Currently, the SKA is expected to
span the frequency range 0.1-25 GHz with capabilities including a wide
...
Repository :
arXiv
Language(s) :
Undetermined
G332.5-5.6, a new Galactic supernova remnant
Description :
We present radio observations of the source G332.5-5.6, a candidate supernova
remnant (SNR). Observations have been performed with the Australia Telescope
Compact Array (ATCA) at two frequencies, at 1.4 and 2.4 GHz. Our results
confirm that G332.5-5.6 is an SNR, with a spectral index equal to -0.7...
Repository :
arXiv
Language(s) :
Undetermined
Radio Observations of Masers in Post-AGB Stars
Description :
We present observations of 86 post-Asymptotic Giant Branch (post-AGB) stars
of OH maser transitions, taken with the Parkes Telescope between September 2002
and August 2003. Post-AGB stars are the precursors of planetary nebulae, which
have a wide range of morphologies that are not well explained. ...
Repository :
arXiv
Language(s) :
Undetermined
OH Maser Observations of Planetary Nebulae Precursors
Description :
We present OH maser observations at 1612, 1665, 1667, and 1720 MHz for 86
post-asymptotic giant branch (post-AGB) stars selected from a survey of 1612
MHz maser sources in the Galactic Plane. The observations were taken with the
Parkes Telescope and the Australia Telescope Compact Array between 20...
Repository :
arXiv
Language(s) :
Undetermined
Radio continuum and HI observations of supernova remnant G296.8-00.3
Description :
We present Australia Telescope Compact Array (ATCA) observations of the
supernova remnant (SNR) G296.8-00.3. A 1.3-GHz continuum image shows the
remnant to have a complex multi-shelled appearance, with an unusual rectangular
strip running through its centre. HI absorption yields a kinematic distan...
Repository :
arXiv
Language(s) :
Undetermined
G309.2-00.6 and jets in supernova remnants
Description :
We present Australia Telescope Compact Array observations of the supernova
remnant (SNR) G309.2-00.6. In a 1.3-GHz continuum image the remnant appears as
a near-circular shell, but with two brightened and distorted arcs of emission
on opposite sides. HI absorption against the SNR yields a distance...
Repository :
arXiv
Language(s) :
Undetermined
A high-resolution radio survey of the Vela supernova remnant
Description :
This paper presents a high-resolution radio continuum (843 MHz) survey of the
Vela supernova remnant. The contrast between the structures in the central
pulsar-powered nebula of the remnant and the synchrotron radiation shell allows
the remnant to be identified morphologically as a member of the c...
Repository :
arXiv
Language(s) :
Undetermined
The clinical value of imaging with antibody to human chorionic gonadotrophin in the detection of residual choriocarcinoma.
Description :
Choriocarcinoma can be imaged by external scintigraphy after intravenous administration of radiolabelled antibody directed against human chorionic gonadotrophin (HCG). The purpose of this study was to investigate whether antibody imaging was sufficiently sensitive and specific to improve the selecti...
Repository :
Europe PubMed Central
Language(s) :
English
Health-related behaviours of people with diabetes and those with cardiometabolic risk factors: results from SHIELD
Description :
Repository :
Europe PubMed Central
Language(s) :
English
Spectropolarimetry of SNR G296.5+10.0
Description :
Radio continuum emission from the supernova remnant G296.5+10.0 was observed
using the Australia Telescope Compact Array. Using a 104 MHz bandwidth split
into 13 x 8 MHz spectral channels, it was possible to produce a pixel-by-pixel
image of Rotation Measure (RM) across the entire remnant. A lack ...
Repository :
arXiv
Language(s) :
Undetermined