61 research outputs found
The Dynamical Structure and Evolution of Giant Molecular Clouds
Get PDFGiant molecular clouds (GMCs) are the sites of star formation in the Galaxy. Many of their properties can be understood in terms of a model in which the GMCs and the star-forming clumps within them are in approximate pressure equilibrium, with turbulent motions treated as a separate pressure component
Plasmodium Helical Interspersed Subtelomeric (PHIST) Proteins, at the Center of Host Cell Remodeling
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Timing and duration of anti–α4β1 integrin treatment after spinal cord injury: effect on therapeutic efficacy
No full textSeptal neurons containing glutamic acid decarboxylase immunoreactivity project to the hippocampal region in the rat brain
No full textT RAINING M ILITARY M EDICS AS C IVILIAN P REHOSPITAL C ARE P ROVIDERS IN S OUTHERN S UDAN
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