Results 1 to 10 of about 200,380 (264)
Symmetric Atom–Atom and Ion–Atom Processes in Stellar Atmospheres [PDF]
We present the results of the influence of two groups of collisional processes (atom–atom and ion–atom) on the optical and kinetic properties of weakly ionized stellar atmospheres layers.
Vladimir A. Srećković +2 more
doaj +2 more sources
Computational Characterization of Astrophysical Species: The Case of Noble Gas Hydride Cations
Theoretical–computational studies together with recent astronomical observations have shown that under extreme conditions in the interstellar medium (ISM), complexes of noble gases may be formed.
María Judit Montes de Oca-Estévez +2 more
doaj +1 more source
Biotransformation of soluble selenite (SeIV) and selenate (SeVI) to biomass-associated Se0 (Bio-Se) provides a solution for mitigating Se pollution coupled to securing scarce element.
M. Sarvajith, Y.V. Nancharaiah
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Stark Width Data for Tb II, Tb III and Tb IV Spectral Lines
A dataset of Stark widths for Tb II, Tb III and Tb IV is presented. To data obtained before, the results of new calculations for 62 Tb III lines from 5d to 6pj(6,j)o, a transition array, have been added.
Milan S. Dimitrijević
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Candida albicans is an opportunistic pathogen causes fungal infections that range from common skin infections to persistent infections through biofilm formation on tissues, implants and life threatening systemic infections.
G. Kiran Kumar Reddy +3 more
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Process Evolution with Atomicity Consistency [PDF]
The processes enacting cross-organizational collaboration continually evolve to adapt to changing business environments. These processes may evolve at any time during collaboration when collaborative organizations should respond timely to critical environment changes. Atomicity is an important requirement for maintaining application consistency.
Chunyang Ye +2 more
openaire +1 more source
Fungal infections: Pathogenesis, antifungals and alternate treatment approaches
Increasing incidence of fungal infections of recent times requires immediate intervention. Fungal infections are seldom construed at initial stages that intensify the severity of infections and complicate the treatment procedures. Fungal pathogens employ
G.Kiran Kumar Reddy +2 more
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Using Griem’s semi-empirical approach, we have calculated the Stark broadening parameters (line widths and shifts) of 35 UV–Blue spectral lines of neutral vanadium (V I).
Cristóbal Colón +3 more
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Ionization of Hydrogen in the Solar Atmosphere
The ionization degree of hydrogen is crucial in the physics of the plasma in the solar chromosphere. It specifically limits the range of plasma temperatures that can be determined from the Hα line.
Jongchul Chae
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Stark Broadening of Zn III Spectral Lines
Stark widths for spectral lines within 24 multiplets of Zn III singlets and triplets have been calculated using modified semiempirical method for an electron density of 1017 cm−3 and temperatures from 5000 K up to 100,000 K.
Milan S. Dimitrijević +1 more
doaj +1 more source

