Results 21 to 30 of about 2,548,043 (302)
Anomalous Fraunhofer Line Profiles [PDF]
Nature, 1962 DURING the spring of 1961 we made observations of the H line of Ca(II) in the spectrum of moonlight, with the view of detecting any luminescent radiation which might have been present. The observations were made with the 50-in. reflector of the University of Padua's Observatory at Asiago.
J. F. GRAINGER, J. RING
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Stark Widths of Yb III and Lu IV Spectral Lines
Atoms, 2019 Rare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broadening data are scarce. For Yb III and Lu IV theoretical as well as experimental data on Stark broadening parameters of spectral lines are absent in the ...
Milan S. Dimitrijević
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Emission Line Profiles from Self-Gravitating Thin Disks [PDF]
, 1994 We have constructed general relativistic models of a stationary, axially symmnetric, Keplerian thin disk around a rotating black hole. We computed profiles of a spectral line, emitted in the inner region of the disk.
Karas, V., Lanza, A., Vokrouhlicky, D.
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Epigenomic profiling of neuroblastoma cell lines [PDF]
Scientific Data, 2020 Abstract Understanding the aberrant transcriptional landscape of neuroblastoma is necessary to provide insight to the underlying influences of the initiation, progression and persistence of this developmental cancer. Here, we present chromatin immunoprecipitation sequencing (ChIP-Seq) data for the oncogenic transcription factors, MYCN
Upton, Kristen +12 more
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Stark Broadening and White Dwarfs
Open Astronomy, 2011 White dwarf and pre-white dwarfs are the best types of stars for the application of Stark broadening research results in astrophysics, since in the atmospheres of these stars physical conditions are very favorable for this line broadening mechanism - in ...
Dimitrijević Milan S. +3 more
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Electron energy-loss spectroscopy of autoionizing states of zinc [PDF]
Serbian Astronomical Journal, 2004 Autoionizing energy-loss spectra of Zn from 10.8 to 12.5 eV, for incident electron energies between 20 and 100 eV, have been recorded at scattering angles from 0° to 10°.
Predojević B. +4 more
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Line-profile variability of EZ CMa [PDF]
Symposium - International Astronomical Union, 1995 CCD spectra for the unusual Wolf-Rayet star EZ CMa (WR6) are presented. The analysis of the profile changes of HeII lines shows a correlation between the gravity center of the line and the skewness (Robert et al. 1992). The fourth moment (kurtosis) changes with phase and looks epoch independent.
L. Georgiev, M. M. Ivanov
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Stark Broadening of Several Ne II, Ne III and O III Spectral Lines for the Stark-B Database
Open Astronomy, 2011 In order to complete Stark broadening data for Ne II and O III lines, needed for analysis of stellar atmospheres, we determined the missing parameters for the broadening by collisions with protons and ionized helium for 15 Ne II and 5 O III multiplets ...
Dimitrijević Milan S. +3 more
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Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Atoms, 2018 Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas.
Milan S. Dimitrijević +5 more
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Line profiles in expanding atmospheres [PDF]
Symposium - International Astronomical Union, 1994 The analysis of the UV resonance transitions of superionized species observed in early-type stars suggests the presence of a high temperature region and an outward flow of matter (Snow & Marlborough 1976).
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