In the next 10-20 years, several observatories will aim to detect the signatures of oxygenic photosynthesis on exoplanets, though targets must be carefully selected. Most known potentially habitable exo-planets orbit cool M-dwarf stars, which have limited emission in the photosynthetically active region of the spectrum (PAR, nm) used by Earth's oxygenic photoautotrophs. Still, recent experiments have shown that model cyanobacteria, algae, and non-vascular plants grow comfortably under simulated M-dwarf light, though vascular plants struggle.
View Article and Find Full Text PDFMost low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict that this FUV radiation produces photodissociation regions (PDRs) on the surfaces of protoplanetary disks around low-mass stars, which affects planet formation within the disks. We report James Webb Space Telescope and Atacama Large Millimeter Array observations of a FUV-irradiated protoplanetary disk in the Orion Nebula.
View Article and Find Full Text PDFCatecholamines mediate the 'fight or flight' response in a wide variety of vertebrates. The endogenous catecholamine adrenaline increases heart rate and contractile strength to raise cardiac output. The increase in contractile force is driven in large part by an increase in myocyte Ca influx on the L-type Ca current (I) during the cardiac action potential (AP).
View Article and Find Full Text PDFWhat Is Known: Spironolactone is used in paediatric patients with heart disease, yet few data are available regarding the impact on potassium supplementation.
Objective: We sought to determine the effect of spironolactone on potassium supplementation in paediatric cardiac intensive care patients.
Methods: A retrospective, propensity matched cohort study was designed.