Centurions and Chieftains : tank sales and British policy towards Israel in the aftermath of the Six Day War

Britain's attempt to distance itself from Israel as London sought to conciliate the Arab world in the aftermath of the Six-Day War has entered the historiography of Anglo-Israeli relations. A neglected aspect of the development of British policy towards Israel has been the intense debates among British decision-makers regarding the supply of tanks to Israel following the 1967 conflict. British reluctance to export the powerful Chieftain tank to Israel stemmed not only from an unwillingness to fuel an arms race in the Middle East, but also from a determination to protect ongoing and extensive British economic interests in the Arab world, especially oil supplies. In keeping with efforts to dissociate itself from Israel, Britain also sought to downplay, and even conceal from the Arab world, ongoing sales of the less sophisticated Centurion tank to Israel. In many ways, British policy towards Israel culminated in the decision during the 1973 Yom Kippur War to maintain an arms embargo to the region which, while not extending to all Arab countries, hit Israel especially hard as it desperately sought ammunition and spares for its Centurion tanks

Britain’s decision to withdraw from the Persian Gulf: a pattern not a puzzle

The reasons for the British decision to withdraw from the Gulf are highly contentious. While some scholars have focused on short-term considerations, especially the devaluation of sterling towards the end of 1967, in the British determination to quit the Gulf, others have concentrated on longer-term trends in British policy-making for the region. This article sides with the latter. Britain's Gulf role came under increasing scrutiny following the 1956 Suez crisis as part of an ongoing debate about the costs and benefits of Britain's Gulf presence. In this sense, British withdrawal fitted into a wider pattern of British decolonisation. By the 1960s, the Treasury, in particular, strongly questioned the necessity and cost-effectiveness of the maintenance of empire in the Gulf to safeguard British economic interests there. Recent interpretations which seek to disaggregate the British decision to leave Southeast Asia from the decision to depart from the Gulf are also questionable. By mid-1967, it had already been determined that Britain would leave both regions by the mid-1970s, the only difference being that this decision was formally announced with respect to Southeast Asia, but not with regard to the Gulf. The devaluation of sterling in November 1967, therefore, merely hastened and facilitated decisions which had already been taken. Despite the end of formal empire in the Gulf, Britain did seek, not always successfully, to preserve its interests into the 1970s and beyond

Priests and politicians: Archbishop Michael Gonzi, Dom Mintoff, and the end of empire in Malta

The political contest in Malta at the end of empire involved not merely the British colonial authorities and emerging nationalists, but also the powerful Catholic Church. Under Archbishop Gonzi’s leadership, the Church took an overtly political stance over the leading issues of the day including integration with the United Kingdom, the declaration of an emergency in 1958, and Malta’s progress towards independence. Invariably, Gonzi and the Church found themselves at loggerheads with the Dom Mintoff and his Malta Labour Party. Despite his uncompromising image, Gonzi in fact demonstrated a flexible turn of mind, not least on the central issue of Maltese independence. Rather than seeking to stand in the way of Malta’s move towards constitutional separation from Britain, the Archbishop set about co-operating with the Nationalist Party of Giorgio Borg Olivier in the interests of securing the position of the Church within an independent Malta. For their part, the British came to accept by the early 1960s the desirability of Maltese self-determination and did not try to use the Church to impede progress towards independence. In the short-term, Gonzi succeeded in protecting the Church during the period of decolonization, but in the longer-term the papacy’s softening of its line on socialism, coupled with the return to power of Mintoff in 1971, saw a sharp decline in the fortunes of the Church and Archbishop Gonzi

The effects of speed cameras: How drivers respond

This study set out to examine the effects and effectiveness of various strategies related to the deployment of speed cameras, and to explore how different types of driver responded to cameras and perceived their operation. Recommendations for best deployment were to be considered. It was carried out between 1993 and 1996 after the Road Traffic Act 1991 authorised the use of automatic speed devices for the detection of offences. A series of 12 surveys arranged in five sets and having some cross-sectional and some longitudinal elements was undertaken together with some depth interviews, and self-report measures predominated. Five police forces helped to set up the research. In total 6879 drivers took part. The particular interventions focused upon comprised camera signing alone; two kinds of publicity campaign linked with speed camera deployment; prosecution following detection by speed camera; and the effects of cameras when first installed and over time.The Department of Environment, Transport and the Regions

On column density thresholds and the star formation rate

We present the results of a numerical study designed to address the question of whether there is a column density threshold for star formation within molecular clouds. We have simulated a large number of different clouds, with volume and column densities spanning a wide range of different values, using a state-of-the-art model for the coupled chemical, thermal and dynamical evolution of the gas. We show that star formation is only possible in regions where the mean (area-averaged) column density exceeds $10^{21} \: {\rm cm^{-2}}$. Within the clouds, we also show that there is a good correlation between the mass of gas above a K-band extinction $A_{\rm K} = 0.8$ and the star formation rate (SFR), in agreement with recent observational work. Previously, this relationship has been explained in terms of a correlation between the SFR and the mass in dense gas. However, we find that this correlation is weaker and more time-dependent than that between the SFR and the column density. In support of previous studies, we argue that dust shielding is the key process: the true correlation is one between the SFR and the mass in cold, well-shielded gas, and the latter correlates better with the column density than the volume density.Comment: 21 pages and 12 figures. Accepted for publication in MNRA

Is atomic carbon a good tracer of molecular gas in metal-poor galaxies?

Carbon monoxide (CO) is widely used as a tracer of molecular hydrogen (H2) in metal-rich galaxies, but is known to become ineffective in low metallicity dwarf galaxies. Atomic carbon has been suggested as a superior tracer of H2 in these metal-poor systems, but its suitability remains unproven. To help us to assess how well atomic carbon traces H2 at low metallicity, we have performed a series of numerical simulations of turbulent molecular clouds that cover a wide range of different metallicities. Our simulations demonstrate that in star-forming clouds, the conversion factor between [CI] emission and H2 mass, $X_{\rm CI}$, scales approximately as $X_{\rm CI} \propto Z^{-1}$. We recover a similar scaling for the CO-to-H2 conversion factor, $X_{\rm CO}$, but find that at this point in the evolution of the clouds, $X_{\rm CO}$ is consistently smaller than $X_{\rm CI}$, by a factor of a few or more. We have also examined how $X_{\rm CI}$ and $X_{\rm CO}$ evolve with time. We find that $X_{\rm CI}$ does not vary strongly with time, demonstrating that atomic carbon remains a good tracer of H2 in metal-poor systems even at times significantly before the onset of star formation. On the other hand, $X_{\rm CO}$ varies very strongly with time in metal-poor clouds, showing that CO does not trace H2 well in starless clouds at low metallicity.Comment: 16 pages, 9 figures. Updated to match the version accepted by MNRAS. The main change from the previous version is a new sub-section (3.6) discussing the possible impact of freeze-out and other processes not included in our numerical simulation