Vaccines against neosporosis: what can we learn from the past studies?

Neospora caninum is an intracellular apicomplexan parasite, which is a leading cause of abortion in cattle; thus neosporosis represents an important veterinary health problem and is of high economic significance. The parasite can infect cattle via trans-placental transmission from an infected cow to its fetus (vertical transmission), or through the oral route via ingestion of food or water contaminated with oocysts that were previously shed with the feces of a canid definitive host (horizontal transmission). Although vaccination was considered a rational strategy to prevent bovine neosporosis, the only commercialized vaccine (Neoguard®) produced ambiguous results with relatively low efficacy, and was recently removed from the market. Therefore, there is a need to develop an efficient vaccine capable of preventing both, the horizontal transmission through infected food or water to a naïve animal as well as the vertical transmission from infected but clinically asymptomatic dams to the fetus. Different vaccine strategies have been investigated, including the use of live attenuated vaccines, killed parasite lysates, total antigens or antigen fractions from killed parasites, and subunit vaccines. The vast majority of experimental studies were performed in mice, and to a certain extent in gerbils, but there is also a large number of investigations that were conducted in cattle and sheep. However, it is difficult to directly compare these studies due to the high variability of the parameters employed. In this review, we will summarize the recent advances made in vaccine development against N. caninum in cattle and in mice and highlight the most important factors, which are likely to influence the degree of protection mediated by vaccination.

Pages & portraits from the past, being the private papers of Sir William Hotham

v.1. Concerning the writer. Early narrative. Under Hood and Nelson. The mutiny at the Nore. Camperdown and after. Life at the Cape. Portraits under George III. The days of Napoleon.--v.2. The days of Napoleon. Portraits after Waterloo. Portraits under George IV. Portraits under William IV. The days of Victoria.

The call from the past, and other stories /

Mode of access: Internet.

A nation trained in arms or a militia? Lessons in war from the past and the present,

"A sequel to the recently published volume, Deductions from the worldwar."--p. viii.

Suggestion from the Past?

Mathematics Subject Classification: 26A33 (main), 35A22, 78A25, 93A30

Strongyloides stercoralis - a Legacy from the Past

The authors present the case of a 65-year-old Caucasian man who had previously lived in Guinea-Bissau. The patient was diagnosed in Portugal with an anti-neutrophil cytoplasmic antibody-associated vasculitis and started on corticosteroids plus cyclophosphamide, with clinical improvement. Some months later, his general status deteriorated, iatrogenic bicytopenia developed and immunosuppressive drugs were tapered. Microbiological tests identified numerous larvae and eggs of Strongyloides stercoralis in various biological samples, and a diagnosis of hyperinfection syndrome was established. The patient was started on antihelminthic drugs but developed septic shock and died. This case highlights a rare and severe complication of immunosuppression in developed countries.

The past and the future fate of the universe and the formation of structure in it

The history and the ultimate future fate of the universe as a whole depend on how much the expansion of the universe is decelerated by its own mass. In particular, whether the expansion of the universe will ever come to a halt can be determined from the past expansion. However, the mass density in the universe does not only govern the expansion history and the curvature of space, but in parallel also regulates the growth of hierarchical structure, including the collapse of material into the dense, virialized regions that we identify with galaxies. Hence, the formation of galaxies and their clustered distribution in space depend not only on the detailed physics of how stars are formed but also on the overall structure of the universe. Recent observational efforts, fueled by new large, ground-based telescopes and the Hubble Space Telescope, combined with theoretical progress, have brought us to the verge of determining the expansion history of the universe and space curvature from direct observation and to linking this to the formation history of galaxies.