Abolishing Australia\u27s Judicially Enacted SUI GENERIS Doctrine of Extended Joint Enterprise

This Article argues that the decision in Miller v The Queen [2016] HCA 30 is supported neither by common law precedent in Australia nor the historical English precedents that informed the development of Australia’s common law doctrines. It is submitted that the majority judgment misquoted old English authorities to try to equate foresight with intention and argues that the High Court of Australia engaged in judicial activism, because its decision rested predominantly on the policy views of the judges. Moreover, it is argued that the case highlighted the urgent need for law reform in Australia. The Article puts forward a theory to demonstrate that treating a person who did not perpetrate the collateral crime or assist or encourage its commission the same as the perpetrator of that collateral crime is unfair and unjust. Therefore, this Article argues that the extended joint enterprise doctrine created in Miller should be rejected in the 21st century

Serendipitous Discovery of An Infrared Bow Shock Near PSR J1549-4848 with Spitzer

We report on the discovery of an infrared cometary nebula around PSR J1549$-$4848 in our Spitzer survey of a few middle-aged radio pulsars. Following the discovery, multi-wavelength imaging and spectroscopic observations of the nebula were carried out. We detected the nebula in Spitzer IRAC 8.0, MIPS 24 and 70 $\mu$m imaging and in Spitzer IRS 7.5--14.4 $\mu$m spectroscopic observations, and also in the WISE all-sky survey at 12 and 22 $\mu$m.These data were analyzed in detail, and we find that the nebula can be described with a standard bow-shock shape, and that its spectrum contains polycyclic aromatic hydrocarbon and H$_2$ emission features. However, it is not certain which object drives the nebula. We analyze the field stars and conclude that none of them can be the associated object because stars with a strong wind or mass ejection that usually produce bow shocks are much brighter than the field stars. The pulsar is approximately 15\arcsec\ away from the region in which the associated object is expected to be located. In order to resolve the discrepancy, we suggest that a highly collimated wind could be emitted from the pulsar and produce the bow shock. X-ray imaging to detect the interaction of the wind with the ambient medium and high-spatial resolution radio imaging to determine the proper motion of the pulsar should be carried out, which will help verify the association of the pulsar with the bow shock nebula.Comment: 9 pages, 5 figures, accepted for publication in Ap