Development and characterization of a self-nano emulsifying drug delivery system (SNEDDS) for Ornidazole to improve solubility and oral bioavailability of BCS class II drugs. [PDF]
Mohite P+12 more
europepmc +1 more source
Herpes Simplex Virus Type 1 (HSV‐1) infection triggers metabolic reprogramming in corneal cells, shifting from mitochondrial respiration to aerobic glycolysis with marked upregulation of Hexokinase‐2 (HK2). This study identifies HK2 as a therapeutic target: inhibiting HK2 with lonidamine significantly reduces viral replication and promotes corneal ...
Dan Jiang+9 more
wiley +1 more source
Male gut microbiome mediates post-mating sexual selection in Drosophila
Maggu K+5 more
europepmc +1 more source
Coenzyme Q10 Enhances Resilience of Mitochondrial-like Membranes Against Amyloidogenic Peptides. [PDF]
Seychell RM+3 more
europepmc +1 more source
Efficient synthesis of N-(ethylcarbamothioyl)-1-naphthamide: X-ray structure, Hirshfeld surface analysis, DFTs, and molecular modelling investigations as selective inhibitor of alkaline phosphatase. [PDF]
Channar PA+9 more
europepmc +1 more source
Bacterial microbiota diversity in sheep milk during refrigerated storage under different processing conditions. [PDF]
Yang X+5 more
europepmc +1 more source
Effects of tillage methods on photosynthetic performance of different functional leaf groups of summer maize in coastal saline-alkali farmland. [PDF]
Li HX+9 more
europepmc +1 more source
Comparative analysis of mouse strains forin vivoreprogramming
Picó S+10 more
europepmc +1 more source
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Our knowledge of the Milky Way has been deeply renewed since a dozen years, following the results of the astrometric satellite HIPPARCOS, and those of large stellar surveys. Many concepts thought to be well established disappeared, to be replaced by others going towards a larger complexity: in particular, the discovery of radial migrations of stars has
Francoise Combes+2 more
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The Structure and Dynamics of the Milky Way Galaxy
2002Now that we have become familiar with the stars, their properties and their motions, and also with the various components of the interstellar medium, we have collected all the “parts” we need in order to consider our Milky Way galaxy. We begin in Sect. 11.1 with the information about the structure of the Milky Way which can be gained from observations ...
Albrecht Unsöld, Bodo Baschek
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