Two Views of ‘Subordination’: the Personal Scope of Employment Discrimination Law in Jivraj v Hashwani

In Jivraj v Hashwani, the Supreme Court considered what requirements are necessary for a relationship to be considered as an employment relationship for the purposes of determining the scope of domestic employment discrimination law. The Court held that an element of subordination was necessary for the relationship to be considered employment under a contract personally to do work. This article discusses what the Court in Jivraj meant by this requirement, contrasting two differing views of subordination. It examines some implications of the decision for the relationship between employment law and anti-discrimination law, and for recent debates on the scope of employment law more generally.

Identification of a general secretory pathway in a human isolate of Burkholderia vietnamiensis (formerly B. cepacia complex genomovar V) that is required for the secretion of hemolysin and phospholipase C activities

Members of the Burkholderia cepacia complex can secrete proteases, lipases, and hemolysins. We report in this study the identification of a general secretory pathway present in a B. vietnamiensis (formerly genomovar V) clinical isolate, which is required for the efficient secretion of phospholipase C and hemolysin activities. Southern blot hybridization experiments revealed that this general secretion pathway is highly conserved among the different genomovars of the B. cepacia complex and is homologous to a similar system described in B. pseudomallei. We also show that this pathway appears not to be necessary for intracellular survival of B. vietnamiensis within Acanthamoeba polyphaga.

A novel calmodulin-like protein from the liver fluke, Fasciola hepatica

An 18.2 kDa protein from the liver fluke, Fasciola hepatica has been identified and characterised. The protein shows strongest sequence similarity to egg antigen proteins from Schistosoma mansoni, Schistosoma japonicum and Clonorchis sinensis. The protein is predicted to adopt a calmodulin-like fold; it thus represents the third calmodulin-like protein to be characterised in F. hepatica and has been named FhCaM3. Compared to the classical calmodulin structure there are some variations. Most noticeably, the central, linker helix is disrupted by a cysteine residue. Alkaline native gel electrophoresis showed that FhCaM3 binds calcium ions. This binding event increases the ability of the protein to bind the hydrophobic fluorescent probe 8-anilinonaphthalene-1-sulphonate, consistent with an increase in surface hydrophobicity as seen in other calmodulins. FhCaM3 binds to the calmodulin antagonists trifluoperazine and W7, but not to the myosin regulatory light chain binding compound praziquantel. Immunolocalisation demonstrated that the protein is found in eggs and vitelline cells. Given the critical role of calcium ions in egg formation and hatching this suggests that FhCaM3 may play a role in calcium signalling in these processes. Consequently the antagonism of FhCaM3 may, potentially, offer a method for inhibiting egg production and thus reducing the spread of infection.

Germany v Italy:The Triumph of Sovereign Immunity over Human Rights Law

This article analyses the doctrine of State immunity within the context of the recent judgment of the International Court of Justice (ICJ) concerning the Jurisdictional Immunities of the State (Germany v Italy: Greece intervening). The object of this article is to explore the implications of the State immunity from foreign judicial proceedings in cases of jus cogens crimes. Challenging the assumption that the law of immunity is merely procedural in nature, this article argues that there can be no immunity in cases of undisputed international crimes.

Review: V. Gessner and D. Nelken (eds.), European Ways of Law (Hart, 2008)

Review of edited collection.

The electron pressure in the outer atmosphere of ∈ Eri (K2 V)

Observations of ? Eri (K2 V) have been made with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. The spectra obtained show a number of emission lines which can be used to determine, or place limits on, the electron density and pressure. Values of the electron pressure are required in order to make quantitative models of the transition region and inner corona from absolute line fluxes, and to constrain semi-empirical models of the chromosphere. Using line flux ratios in Si II and O IV a mean electron pressure of P = NT = 4.8 × 10 cm K is derived. This value is compatible with the lower and upper limits to P found from flux ratios in C III, O V and Fe XII. Some inconsistencies which may be because of small uncertainties in the atomic data used are discussed.

Modelling the chromosphere and transition region of ε Eri (K2 V)

Measurements of ultraviolet line fluxes from Space Telescope Imaging Spectrograph and Far-Ultraviolet Spectroscopic Explorer spectra of the K2-dwarf e Eri are reported. These are used to develop new emission measure distributions and semi-empirical atmospheric models for the chromosphere and lower transition region of the star. These models are the most detailed constructed to date for a main-sequence star other than the Sun. New ionization balance calculations, which account for the effect of finite density on dielectronic recombination rates, are presented for carbon, nitrogen, oxygen and silicon. The results of these calculations are significantly different from the standard Arnaud & Rothenflug ion balance, particularly for alkali-like ions. The new atmospheric models are used to place constraints on possible first ionization potential (FIP)-related abundance variations in the lower atmosphere and to discuss limitations of single-component models for the interpretation of certain optically thick line fluxes. © 2005 RAS.

On the filling factor of emitting material in the upper atmosphere of ε Eri (K2 V)

The emission measure distribution in the upper transition region and corona of e Eri is derived from observed emission-line fluxes. Theoretical emission measure distributions are calculated assuming that the radiation losses are balanced by the net conductive flux. We discuss how the area factor of the emitting regions as a function of temperature can be derived from a comparison between these emission measure distributions. It is found that the filling factor varies from ~0.2 in the mid-transition region to ~1.0 in the inner corona. The sensitivity of these results to the adopted ion fractions, the iron abundance and other parameters is discussed. The area factors found are qualitatively similar to the observed structure of the solar atmosphere, and can be used to constrain two-component models of the chromosphere. Given further observations, the method could be applied to investigate the trends in filling factors with indicators of stellar activity.