Progress in medical aspects of liver disease

Recent advances in the medical aspects of liver disease are reviewed,  especially in the areas of viral hepatitis, chronic aggressive hepatitis and  cirrhosis

Chlorothiazide- its mode of action and its use in patients with oedema

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Toxoplasmosis in the adult

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Observations on a family with chronic hyperbilirubinaemia

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A clinical trial of Carbutamide (BZ 55) in diabetics admitted to hospital

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Liver Function in the Pig

The assessment of function of the isolated perfused liver remains complex. Much of this problem relates to an inability to compare function in vitro with that in vivo, because of a lack of knowledge of hepatic blood flow. This article documents measurement of total hepatic and portal blood flow in vivo in pigs, by means of the dye clearance method. The effects of starvation, glucose administration and anaesthesia are noted. Although these techniques are simple and may be performed in the awake animal, there are wide variations in values which would necessitate individual flow readings being obtained for any comparative study.S. Afr. Med. J., 48, 1197 (1974)

Congenital hepatic fibrosis: A case report and family study

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Hypokalaemia during extracorporeal circulation - An Eperimental study

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Measuring Black Hole Spin in OJ287

We model the binary black hole system OJ287 as a spinning primary and a non-spinning secondary. It is assumed that the primary has an accretion disk which is impacted by the secondary at specific times. These times are identified as major outbursts in the light curve of OJ287. This identification allows an exact solution of the orbit, with very tight error limits. Nine outbursts from both the historical photographic records as well as from recent photometric measurements have been used as fixed points of the solution: 1913, 1947, 1957, 1973, 1983, 1984, 1995, 2005 and 2007 outbursts. This allows the determination of eight parameters of the orbit. Most interesting of these are the primary mass of $1.84\cdot 10^{10} M_\odot$, the secondary mass $1.46\cdot 10^{8} M_\odot$, major axis precession rate $39^\circ.1$ per period, and the eccentricity of the orbit 0.70. The dimensionless spin parameter is $0.28\:\pm\:0.01$ (1 sigma). The last parameter will be more tightly constrained in 2015 when the next outburst is due. The outburst should begin on 15 December 2015 if the spin value is in the middle of this range, on 3 January 2016 if the spin is 0.25, and on 26 November 2015 if the spin is 0.31. We have also tested the possibility that the quadrupole term in the Post Newtonian equations of motion does not exactly follow Einstein's theory: a parameter $q$ is introduced as one of the 8 parameters. Its value is within 30% (1 sigma) of the Einstein's value $q = 1$. This supports the $no-hair theorem$ of black holes within the achievable precision. We have also measured the loss of orbital energy due to gravitational waves. The loss rate is found to agree with Einstein's value with the accuracy of 2% (1 sigma).Comment: 12 pages, 4 figures, IAU26

Advances in multispectral and hyperspectral imaging for archaeology and art conservation

Multispectral imaging has been applied to the field of art conservation and art history since the early 1990s. It is attractive as a noninvasive imaging technique because it is fast and hence capable of imaging large areas of an object giving both spatial and spectral information. This paper gives an overview of the different instrumental designs, image processing techniques and various applications of multispectral and hyperspectral imaging to art conservation, art history and archaeology. Recent advances in the development of remote and versatile multispectral and hyperspectral imaging as well as techniques in pigment identification will be presented. Future prospects including combination of spectral imaging with other noninvasive imaging and analytical techniques will be discussed