German Mission in Abyssinia: Wilhelm Staiger from Baden, 1835–1904

This article deals with the story of the Christian mission among the Jews of Ethiopia during the 1860s as related in the memoirs of the German missionary, Wilhelm Staiger, publicised here for the first time. Staiger who had, together with scores of other European missionaries, become caught up in the political turmoil between Great Britain and Teodoros, King of Ethiopia, describes the affair in the first person

Scleromyxedema with systemic involvement mimics rheumatic diseases

Scleromyxedema is an infiltrative skin disease produced by hyaluronic acid deposition in the dermis. A benign monoclonal gammopathy is usually present. We report 2 patients with scleromyxedema and systemic illnesses. Both patients had muscle weakness, dysphagia, and weight loss in addition to the skin changes. One also had sclerodactyly, telangiectasias, and Raynaud's phenomenon. Scleromyxedema with systemic involvement may mimic rheumatic diseases.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/37776/1/1780290716_ftp.pd

Swift X-Ray Observations of Classical Novae. II. The Super Soft Source sample

The Swift GRB satellite is an excellent facility for studying novae. Its rapid response time and sensitive X-ray detector provides an unparalleled opportunity to investigate the previously poorly sampled evolution of novae in the X-ray regime. This paper presents Swift observations of 52 Galactic/Magellanic Cloud novae. We included the XRT (0.3-10 keV) X-ray instrument count rates and the UVOT (1700-8000 Angstroms) filter photometry. Also included in the analysis are the publicly available pointed observations of 10 additional novae the X-ray archives. This is the largest X-ray sample of Galactic/Magellanic Cloud novae yet assembled and consists of 26 novae with super soft X-ray emission, 19 from Swift observations. The data set shows that the faster novae have an early hard X-ray phase that is usually missing in slower novae. The Super Soft X-ray phase occurs earlier and does not last as long in fast novae compared to slower novae. All the Swift novae with sufficient observations show that novae are highly variable with rapid variability and different periodicities. In the majority of cases, nuclear burning ceases less than 3 years after the outburst begins. Previous relationships, such as the nuclear burning duration vs. t_2 or the expansion velocity of the eject and nuclear burning duration vs. the orbital period, are shown to be poorly correlated with the full sample indicating that additional factors beyond the white dwarf mass and binary separation play important roles in the evolution of a nova outburst. Finally, we confirm two optical phenomena that are correlated with strong, soft X-ray emission which can be used to further increase the efficiency of X-ray campaigns.Comment: Accepted to ApJ Supplements. Full data for Table 2 and Figure 17 available in the electronic edition. New version of the previously posted paper since the earlier version was all set in landscape mod

Uncovering Ubiquitin and Ubiquitin-like Signaling Networks

Microscopic imaging and technolog

Management of malignancy-induced, life-threatening hypoxemic respiratory failure using a self-expanding Y stent

We present the case of a young woman transferred to our center with acute hypoxic respiratory failure due to an obstructing subcarinal mass. We review the management and rationale of this respiratory failure at different stages of her hospital course. We describe the approach and rationale in both the intensive care unit as well as the bronchoscopy suite. Finally, we discuss how the use of a novel hybrid Y stent effectively palliated her symptoms