Publications by authors named "A RICCA"

Molecular dynamics simulations were performed to characterize reaction products, resulting from solar wind irradiation, namely, H, of methane and methane-water ices. In our approach, we used seven 0.829 keV H (total energy of 5.

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The effects of cosmic-ray bombardment of chiral molecules in the interstellar medium are simulated in the laboratory by performing radiolysis experiments of pure α-pinene ices at four different temperatures. The identification and significance of α-pinene have not been fully understood because of the insufficient amount of spectral information of these compounds at low temperatures. A comparison of the temperature dependence of the mid-infrared spectra of pure α-pinene ices before and after irradiation its irradiation by 61.

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Article Synopsis
  • Research shows that healthcare delivery in the U.S. is inconsistent and unequal, particularly impacting mental illness management, life expectancy, mortality rates, and access due to racial and cultural disparities.
  • The situation in New Mexico illustrates the complex challenges residents face, especially regarding liver transplantation.
  • The new liver transplantation system introduced in 2020 by the OPTN may help reduce these inequalities, leading to cautious optimism for better access to transplants for New Mexicans in the future.
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Mitral regurgitation (MR) results from retrograde blood flow from the left ventricle to the left atrium. Common etiologies of acute severe MR include papillary muscle rupture from myocardial infarction, leaflet perforation in infective endocarditis, chordal rupture (pop) in myxomatous valve disease, acute rheumatic fever with carditis, or functional MR due to cardiomyopathies, myocarditis or Takotsubo cardiomyopathy. Here, we present an unusual case of acute severe MR due to ruptured chordae tendineae likely secondary to degenerative valve disease.

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Most 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.

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