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Cleto Alvarez-Aguilar,Maria Lucia Enrí,quez-Ramí,rez,Benigno Figueroa-Nuñ,ez,Anel Gó,mez-Garcí,a,Ernesto Rodrí,guez-Ayala,Cristina Morá,n-Moguel,Victor Manuel 생화학분자생물학회 2007 Experimental and molecular medicine Vol.39 No.3
Metabolic Syndrome (MS) is recognized as a cluster of cardiovascular risk factors. All components of MS have a genetic base. Genes of the renin angiotensin system are potential candidate genes for MS. We investigated whether angiotensin converting en-zyme (ACE) gene polymorphism increases suscep-tibility to MS as an entity in a Mexican population. In a cross-sectional study, 514 individuals were studied including 245 patients with MS and 269 subjects without MS criteria. ACE gene polymorphism was detected using PCR. MS was defined according to The National Cholesterol Education Program Expert Blood Cholesterol in Adults (Adult Treatment Panel III) criteria, except that the raised fasting plasma glucose ≥100 mg/dl criterion for identification of intolerance fasting glucose was modified in accordance with the suggestion of the American Diabetes Association. Patients with MS were sig - nificantly different from subjects without MS in relation to mean body mass index (BMI), waist circumference (WC), systolic blood pressure, diastolic blood pressure, glucose, total cholesterol (C), triglycerides, HDL-C, and LDL-C (P<0.0001). The differences in the mean BMI, WC, glucose, total cholesterol, triglycerides, LDL-C, and HDL-C were maintained in patients with the MS and DD genotypes (P<0.01). The DD genotype was strongly asso - ciated with MS (adjusted OR = 5.48, 95% CI 3.20-9.38, P<0.0001). We concluded that the DD genotype increases susceptibility to MS in a Mexican pop - ulation. These results indicate that pharmacological and non-pharmacological treatment and a reduction in body fat will have important therapeutic im - plications in this disease.
The variability of magnetic activity in solar‐type stars
Fabbian, D.,Simoniello, R.,Collet, R.,Criscuoli, S.,Korhonen, H.,Krivova, N. A.,Olá,h, K.,Jouve, L.,Solanki, S. K.,Alvarado‐,Gó,mez, J. D.,Booth, R.,Garcí,a, R. A.,Lehtinen, J. WILEY‐VCH Verlag GmbH Co. KGaA 2017 Astronomische Nachrichten Vol.338 No.7
<P>This article reviews the current knowledge and status of investigations on the variable magnetic activity of cool stars. We discuss the Sun in the context of solar‐type stars, highlighting peculiarities and common features in terms of its magnetic activity and variability over different time scales. We examine how both theory and observations are providing new clues about the main physical processes that generate magnetic fields in the interior of cool stars, as well as about those that lead to evolving stellar surface magnetism and varying chromospheric and coronal phenomena. We then proceed to discuss the relations between stellar age, rotation, and activity throughout the evolution of cool stars. Finally, we touch upon the importance of understanding stellar magnetism also in view of its effect on planetary environments.</P>