Results 11 to 20 of about 8,079,770 (310)

Natural line profile asymmetry

open access: yesPhysica Scripta, 2022
Abstract The paper discusses the line profile asymmetry of the photon scattering process that arises naturally in quantum electrodynamics (QED). Based on precision spectroscopic experiments conducted on hydrogen atoms, we focus our attention on the two-photon 1s − 2s transition.
A Anikin, T Zalialiutdinov, D Solovyev
openaire   +2 more sources

Line Profile Variations in AGN [PDF]

open access: yesInternational Astronomical Union Colloquium, 1994
AbstractLine-profile variations in the Seyfert galaxies NGC 5548 and NGC 4593 are discussed. The variations of individual line segments are different from line to line and from outburst to outburst.
W. Kollatschny, M. Dietrich
openaire   +2 more sources

Diffraction Line Profiles in the Rietveld Method

open access: yes, 2020
The present work traces the evolution of the modeling of the diffraction line profiles in the Rietveld method, starting from the early and most schematic description with Gaussian curves to the mos...
P. Scardi
semanticscholar   +1 more source

Stark Broadening of N VI Spectral Lines

open access: yesUniverse, 2023
Stark broadening parameters, line widths and shifts, for 15 N VI multiplets are calculated using semiclassical perturbation theory for temperatures from 50,000 K to 2,000,000 K, and perturber density of 1016 cm−3. As perturbers have been taken electrons,
Milan S. Dimitrijević   +2 more
doaj   +1 more source

What Sets the Line Profiles in Tidal Disruption Events? [PDF]

open access: yes, 2017
We investigate line formation in gas that is outflowing and optically thick to electron scattering, as may be expected following the tidal disruption of a star by a supermassive black hole.
Nathaniel Roth, D. Kasen
semanticscholar   +1 more source

Measured Stark widths and shifts in the O IV spectrum [PDF]

open access: yesSerbian Astronomical Journal, 2003
Stark widths (W) and shifts (d) of 5 prominent triply ionized oxygen (O IV) spectral lines in 3 multiplets have been measured in oxygen plasma at 42 000 K electron temperature using a linear, low-pressure, pulsed arc discharge as an optically thin plasma
Đeniže Stevan   +3 more
doaj   +1 more source

Non-Maxwellian Analysis of the Transition-region Line Profiles Observed by the Interface Region Imaging Spectrograph [PDF]

open access: yes, 2017
We investigate the nature of the spectral line profiles for transition-region (TR) ions observed with the Interface Region Imaging Spectrograph (IRIS).
J. Dudík   +4 more
semanticscholar   +1 more source

Extreme Quasars as Distance Indicators in Cosmology

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Quasars accreting matter at very high rates (known as extreme Population A [xA] quasars, possibly associated with super-Eddington accreting massive black holes) may provide a new class of distance indicators covering cosmic epochs from present day up to ...
Deborah Dultzin   +10 more
doaj   +1 more source

Line Profiles in the Bulge of NGC7217 [PDF]

open access: yesSymposium - International Astronomical Union, 1993
Line-of-sight velocity distributions are becoming increasingly important for our understanding of galactic structure. We present results obtained for the bulge of NGC7217 with a new deconvolution technique.
Konrad Kuijken, Michael R. Merrifield
openaire   +1 more source

First evidence of non-Gaussian solar flare EUV spectral line profiles and accelerated non-thermal ion motion [PDF]

open access: yes, 2016
The properties of solar flare plasma can be determined from the observation of optically thin lines. The emitting ion distribution determines the shape of the line, with an isothermal Maxwellian ion distribution producing a Gaussian profile. Non-Gaussian
N. Jeffrey, L. Fletcher, N. Labrosse
semanticscholar   +1 more source

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