Results 31 to 40 of about 999,597 (267)
Correcting the Input Data for Calculating the Asymmetry of Hydrogenic Spectral Lines in Plasmas
We provide corrections to the data in Sholin’s tables from his paper in Optics and Spectroscopy 26 (1969) 27. Since his data was used numerous times by various authors to calculate the asymmetry of hydrogenic spectral lines in plasmas, our corrections ...
Paul Sanders, Eugene Oks
doaj +1 more source
Stark Broadening of O I Spectral Lines
We do not know a priori chemical composition of a star. However, with more high resolution spectra becoming more abundant thanks to the development of space-born observations, atomic data including Stark broadening parameters for various spectral lines ...
Milan S. Dimitrijević +1 more
doaj +1 more source
Origin and properties of non-Lorentzian spectral lines in linear chains of nanospheres are discussed. The lines are shown to be super-exponentially narrow with the characteristic width proportional to exp[-C(h/a)^3] where C is a numerical constant, h the
Bohren C F +6 more
core +2 more sources
Molecular line survey of the high-mass star-forming region NGC 6334I with Herschel/HIFI and the SMA [PDF]
We aim at deriving the molecular abundances and temperatures of the hot molecular cores in the high-mass star-forming region NGC 6334I and consequently deriving their physical and astrochemical conditions. In the framework of the Herschel guaranteed time
A. Schmiedeke +62 more
core +5 more sources
Photometric redshifts from reconstructed QSO templates [PDF]
From SDSS commissioning photometric and spectroscopic data, we investigate the utility of photometric redshift techniques to the task of estimating QSO redshifts. We consider empirical methods (e.g.
Alexander S. Szalay +21 more
core +2 more sources
Energy Levels and Transition Data of Cs VI
Previously reported atomic data (spectral lines, wavelengths, energy levels, and transition probabilities) were collected and systematically analyzed for Cs VI.
Abid Husain, Haris Kunari, Tauheed Ahmad
doaj +1 more source
The HIFI spectral survey of AFGL 2591 (CHESS). II. Summary of the survey [PDF]
This paper presents the richness of submillimeter spectral features in the high-mass star forming region AFGL 2591. As part of the CHESS (Chemical Herschel Survey of Star Forming Regions) Key Programme, AFGL 2591 was observed by the Herschel/HIFI ...
Ceccarelli, C. +5 more
core +5 more sources
ABSTRACT Pediatric gastroenteropancreatic neuroendocrine neoplasms (GEP‐NENs) are extremely rare and clinically heterogeneous. Management has largely been extrapolated from adult practice. This European Standard Clinical Practice Guideline (ESCP), developed by the EXPeRT network in collaboration with adult NEN experts, provides (adult) evidence ...
Michaela Kuhlen +23 more
wiley +1 more source
LAWS IN BEHAVIOUR OF NonLTE EFFECTS FOR THE NaI AND Mgl ATOMS FOR K - A STARS
NonLTE calculations for the Nal and Mgl atoms were performed for model atmospheres of Tef= 4000 - 12000K. logg = 0.0 - 4.5, [NI/H] = 0.5- (-4). Departures from LTE result in strengthening the Nal spectral lines and weakening the Mgl ones.
L. I. Mashonkina +2 more
doaj +1 more source
Numerical modeling of radiation heat exchange in combustion chambers and heat exchangers of power installations [PDF]
The application of numerical modeling is considered to solve the problems of radiation heat exchange in structurally inhomogeneous two-phase media which are realized during the combustion of fuel in boiler units atmospheric emissions from air carriers ...
Moskalenko Nikolay +2 more
doaj +1 more source

