To send content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about sending content to .
To send content items to your Kindle, first ensure firstname.lastname@example.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about sending to your Kindle.
Note you can select to send to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be sent to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
This paper is concerned with East Africans’ perceptions of the intersection between their own, highly charged and contested, local histories, and the global past, as well as their place in it. The two case studies on which the paper is based – Eritrea and Uganda – have much in common in terms of recent history, not least in their experience of prolonged violence, and thus taken together they elucidate distinctive characteristics. Yet they also illustrate broader phenomena. On one level, particular interpretations of local history – both the deeper, precolonial past and the more recent, twentieth-century past – are utilised to critique the flow of global history, as well as the impositions of globalisation, and to emphasise the bitter experience of marginality and lack of agency. At the same time, the global past – conceptualised as the evolution of an intrusive, imperialist, hypocritical global order imposed by foreigners, usually Western in provenance – is seen as omnipresent and pervasive, and thus the arguments made around marginality serve to remind us, paradoxically, how central these communities are (or should be) to the framing of global history.
In Canada, recreational use of cannabis was legalized in October 2018. This policy change along with recent publications evaluating the efficacy of cannabis for the medical treatment of epilepsy and media awareness about its use have increased the public interest about this agent. The Canadian League Against Epilepsy Medical Therapeutics Committee, along with a multidisciplinary group of experts and Canadian Epilepsy Alliance representatives, has developed a position statement about the use of medical cannabis for epilepsy. This article addresses the current Canadian legal framework, recent publications about its efficacy and safety profile, and our understanding of the clinical issues that should be considered when contemplating cannabis use for medical purposes.
The Korean VLBI Network (KVN) is a unique millimeter VLBI system which is consisted of three 21 m telescopes with relatively short baselines. We present the preliminary results of simultaneous monitoring observations of the 22.2 GHz H2O and 43.1/42.8/86.2/129.3 GHz SiO masers based on the KVN Key Science Project (KSP). We obtained the astrometrically registered maps of the H2O and SiO masers toward nine evolved stars using the source frequency phase referencing method (SFPR). The SFPR maps of the H2O and SiO masers enabled us to investigate the spatial structure and kinematics from the SiO to H2O maser regions including the development of an outward motion from the ring-like or elliptical structures of SiO masers to the asymmetric structures of the 22.2 GHz H2O maser features. In particular, the 86.2/129.3 GHz SiO (v=1, J=2–1 and J=3–2) masers were clearly imaged toward several objects for the first time. The SiO v=1, J=3–2 maser shows different distributions compared to those of the SiO v=1, 2, J=1–0 and v=1, J=2–1 masers implying a different physical condition.
Variable OH/IR stars are Asymptotic Giant Branch (AGB) stars with an optically thick circumstellar envelope that emit strong OH 1612 MHz emission. They are commonly observed throughout the Galaxy but also in the LMC and SMC. Hence, the precise inference of the distances of these stars will ultimately result in better constraints on their mass range in different metallicity environments. Through a multi-year long-term monitoring program at the Nancay Radio telescope (NRT) and a complementary high-sensitivity mapping campaign at the eMERLIN and JVLA to measure precisely the angular diameter of the envelopes, we have been re-exploring distance determination through the phase-lag method for a sample of stars, in order to refine the poorly-constrained distances of some and infer the currently unknown distances of others. We present here an update of this project.
W49 A is a star-forming region (SFR) found in the constellation of Aquila. It contains 3 active regions: W49 North (W49 N), W49 South West (W49 SW) and W49 South (W49 S). We present preliminary results from two epochs (e-)MERLIN observations of all ground-state OH masers towards the star-forming region (SFR) complex W49 A. The first epoch of observations was done in full-polarization mode with MERLIN in 2005 while the second epoch was obtained only in dual circular polarization during the test observations of the upgraded e-MERLIN in 2013. The overall maser spatial distributions in both epochs are in good agreement. We found several new high velocity maser features up to +34 km s−1 and −28 km s−1. The magnetic field strengths are between 1.1 to 10.8 mG. All three sources show evidence of magnetic field reversal.
Theoretical simulations have shown that magnetic fields play an important role in massive star formation: they can suppress fragmentation in the star forming cloud, enhance accretion via disc and regulate outflows and jets. However, models require specific magnetic configurations and need more observational constraints to properly test the impact of magnetic fields. We investigate the magnetic field structure of the massive protostar IRAS18089-1732, analysing 6.7 GHz CH3OH maser MERLIN observations. IRAS18089-1732 is a well studied high mass protostar, showing a hot core chemistry, an accretion disc and a bipolar outflow. An ordered magnetic field oriented around its disc has been detected from previous observations of polarised dust. This gives us the chance to investigate how the magnetic field at the small scale probed by masers relates to the large scale field probed by the dust.
Outstanding problems concerning mass-loss from evolved stars include initial wind acceleration and what determines the clumping scale. Reconstructing physical conditions from maser data has been highly uncertain due to the exponential amplification. ALMA and e-MERLIN now provide image cubes for five H2O maser transitions around VY CMa, at spatial resolutions comparable to the size of individual clouds or better, covering excitation states from 204 to 2360 K. We use the model of Gray et al. 2016, to constrain variations of number density and temperature on scales of a few au, an order of magnitude finer than is possible with thermal lines, comparable to individual cloud sizes or locally almost homogeneous regions. We compare results with the models of Decin et al. 2006 and Matsuura et al. 2014 for the circumstellar envelope of VY CMa; in later work this will be extended to other maser sources.
The surface waters of the Southern Ocean play a key role in the global climate and carbon cycles by promoting growth of some of the world’s largest phytoplankton blooms. Several studies have emphasized the importance of glacial and sediment inputs of Fe that fuel the primary production of the Fe-limited Southern Ocean. Although the fertile surface waters along the shelf of the western Antarctic Peninsula (WAP) are influenced by large inputs of freshwater, this freshwater may take multiple pathways (e.g. calving, streams, groundwater discharge) with different degrees of water-rock interactions leading to variable Fe flux to coastal waters. During the summers of 2012–13 and 2013–14, seawater samples were collected along the WAP, near Anvers Island, to observe water column dynamics in nearshore and offshore waters. Tracers (223,224Ra, 222Rn, 18O, 2H) were used to evaluate the source and transport of water and nutrients in coastal fjords and across the shelf. Coastal waters are compared across two field seasons, with increased freshwater observed during 2014. Horizontal mixing rates of water masses along the WAP ranged from 110–3600 m2 s-1. These mixing rates suggest a rapid transport mechanism for moving meltwater offshore.
St Andrews was of tremendous significance in medieval Scotland. Its importance remains readily apparent in the buildings which cluster the rocky promontory jutting out into the North Sea: the towers and walls of cathedral, castle and university provide reminders of the status and wealth of the city in the Middle Ages. As a centre of earthly and spiritual government, as the place of veneration forScotland's patron saint and as an ancient seat of learning, St Andrews was the ecclesiastical capital of Scotland. This volume provides the first full study of this special and multi-faceted centre throughout its golden age. The fourteen chapters use St Andrews as a focus for the discussion of multiple aspects of medieval life in Scotland. They examine church, spirituality, urban society andlearning in a specific context from the seventh to the sixteenth century, allowing for the consideration of St Andrews alongside other great religious and political centres of medieval Europe.
Michael Brown is Professor of Medieval Scottish History, University of St Andrews; Katie Stevenson is Keeper of Scottish History and Archaeology, National Museums Scotland and Senior Lecturer in Late Medieval History, University of St Andrews.
Contributors: Michael Brown, Ian Campbell, David Ditchburn, Elizabeth Ewan, Richard Fawcett, Derek Hall, Matthew Hammond, Julian Luxford, Roger Mason, Norman Reid, Bess Rhodes, Catherine Smith, Katie Stevenson, Simon Taylor, Tom Turpie.
This book is the first major study in several decades to consider Uganda as a nation, from its precolonial roots to the present day. Here, Richard J. Reid examines the political, economic, and social history of Uganda, providing a unique and wide-ranging examination of its turbulent and dynamic past for all those studying Uganda's place in African history and African politics. Reid identifies and examines key points of rupture and transition in Uganda's history, emphasising dramatic political and social change in the precolonial era, especially during the nineteenth century, and he also examines the continuing repercussions of these developments in the colonial and postcolonial periods. By considering the ways in which historical culture and consciousness has been ever present - in political discourse, art and literature, and social relationships - Reid defines the true extent of Uganda's viable national history.