Keele University

About: Keele University is a education organization based out in Newcastle-under-Lyme, United Kingdom. It is known for research contribution in the topics: Population & Stars. The organization has 11318 authors who have published 26323 publications receiving 894671 citations. The organization is also known as: Keele University.

Heavy Metal Poisoning and Cardiovascular Disease

Abstract: Cardiovascular disease (CVD) is an increasing world health problem. Traditional risk factors fail to account for all deaths from CVD. It is mainly the environmental, dietary and lifestyle behavioral factors that are the control keys in the progress of this disease. The potential association between chronic heavy metal exposure, like arsenic, lead, cadmium, mercury, and CVD has been less well defined. The mechanism through which heavy metals act to increase cardiovascular risk factors may act still remains unknown, although impaired antioxidants metabolism and oxidative stress may play a role. However, the exact mechanism of CVD induced by heavy metals deserves further investigation either through animal experiments or through molecular and cellular studies. Furthermore, large-scale prospective studies with follow up on general populations using appropriate biomarkers and cardiovascular endpoints might be recommended to identify the factors that predispose to heavy metals toxicity in CVD. In this review, we will give a brief summary of heavy metals homeostasis, followed by a description of the available evidence for their link with CVD and the proposed mechanisms of action by which their toxic effects might be explained. Finally, suspected interactions between genetic, nutritional and environmental factors are discussed.

Growth Hormone and Pituitary Radiotherapy, But Not Serum Insulin-Like Growth Factor-I Concentrations, Predict Excess Mortality in Patients with Acromegaly

Abstract: Increased mortality in patients with acromegaly has been confirmed in a number of retrospective studies, but causative factors and relationship to serum IGF-I remain uncertain. The West Midlands Pituitary database contains details of 419 patients (241 female) with acromegaly. Serum IGF-I data from the Regional Endocrine Laboratory were available for 360 patients (86%). At diagnosis, mean age was 47 yr (range, 12-84) and mean duration of follow-up was 13 yr (0.5-48). Sixty-one percent were treated by surgery and 39% by nonsurgical means. Radiotherapy was used alone or as adjuvant therapy in 50%. All patients were registered with the Office of National Statistics to obtain information on deaths. At the date of analysis (31 December 2001), 95 of the 419 patients had died (43 males), giving a standardized mortality ratio of 1.26 [confidence interval (CI), 1.03-1.54; P = 0.046]. After controlling for age and sex, data indicated that mortality was increased in subjects with posttreatment GH levels more than 2 micro g/liter, compared with those with levels less than 2 micro g/liter [ratio of mortality rates (RR), 1.55 (range, 0.97-2.50); P = 0.068]. By contrast, a much smaller increase was observed for subjects with elevated posttreatment IGF-I levels compared with those with normal levels [RR, 1.20 (range, 0.71-2.03); P = 0.50]. Treatment with radiotherapy was associated with increased mortality [RR, 1.67 (range, 1.09-2.56); P = 0.018], with cerebrovascular disease the predominant cause of death [standardized mortality ratio, 4.42 (range, 2.71-7.22); P = 0.005]. These results confirm the increased mortality in acromegaly and suggest that reduction of GH levels to less than 2 micro g/liter is beneficial in terms of improving long-term outcome. The sole use of IGF-I as a marker for effective treatment of acromegaly is not justified by this data. This study also highlights the potential deleterious effect of radiotherapy.

The Kepler characterization of the variability among A- and F-type stars I. General overview

Abstract: Context. The Kepler spacecraft is providing time series of photometric data with micromagnitude precision for hundreds of A-F type stars. Aims. We present a first general characterization of the pulsational behaviour of A-F type stars as observed in the Kepler light curves of a sample of 750 candidate A-F type stars, and observationally investigate the relation between γ Doradus (γ Dor), δ Scuti (δ Sct), and hybrid stars. Methods. We compile a database of physical parameters for the sample stars from the literature and new ground-based observations. We analyse the Kepler light curve of each star and extract the pulsational frequencies using different frequency analysis methods. We construct two new observables, “energy ”a nd “efficiency”, related to the driving energy of the pulsation mode and the convective efficiency of the outer convective zone, respectively. Results. We propose three main groups to describe the observed variety in pulsating A-F type stars: γ Dor, δ Sct, and hybrid stars. We assign 63% of our sample to one of the three groups, and identify the remaining part as rotationally modulated/active stars, binaries, stars of different spectral type, or stars that show no clear periodic variability. 23% of the stars (171 stars) are hybrid stars, which is a much higher fraction than what has been observed before. We characterize for the first time a large number of A-F type stars (475 stars) in terms of number of detected frequencies, frequency range, and typical pulsation amplitudes. The majority of hybrid stars show frequencies with all kinds of periodicities within the γ Dor and δ Sct range, also between 5 and 10 d −1 , which is a challenge for the current models. We find indications for the existence of δ Sct and γ Dor stars beyond the edges of the current observational instability strips. The hybrid stars occupy the entire region within the δ Sct and γ Dor instability strips and beyond. Non-variable stars seem to exist within the instability strips. The location of γ Dor and δ Sct classes in the (Teff ,l ogg)-diagram has been extended. We investigate two newly constructed variables, “efficiency ”a nd “energy”, as a means to explore the relation between γ Dor and δ Sct stars. Conclusions. Our results suggest a revision of the current observational instability strips of δ Sct and γ Dor stars and imply an investigation of pulsation mechanisms to supplement the κ mechanism and convective blocking effect to drive hybrid pulsations. Accurate physical parameters for all stars are needed to confirm these findings.