Temperature Dependence of Emission Line Widths from Semiconductor Nanocrystals Reveals Vibronic Contributions to Line Broadening Processes

2017 ◽  
Vol 121 (51) ◽  
pp. 28537-28545 ◽  
Author(s):  
Timothy G. Mack ◽  
Lakshay Jethi ◽  
Patanjali Kambhampati
Keyword(s):  
Emission Line ◽  
Temperature Dependence ◽  
Semiconductor Nanocrystals ◽  
Line Broadening ◽  
Line Widths

scholarly journals Toward Engineering Intrinsic Line Widths and Line Broadening in Perovskite Nanoplatelets

ACS Nano ◽  
2021 ◽  
Vol 15 (4) ◽  
pp. 6499-6506
Author(s):  
Albert Liu ◽  
Gabriel Nagamine ◽  
Luiz G. Bonato ◽  
Diogo B. Almeida ◽  
Luiz F. Zagonel ◽  
...  
Keyword(s):  
Line Broadening ◽  
Line Widths

scholarly journals Upper limits on the mass of supermassive black holes from STIS archival data

2007 ◽  
Vol 3 (S245) ◽  
pp. 233-234
Author(s):  
A. Beifiori ◽  
E. M. Corsini ◽  
E. Dalla Bontà ◽  
A. Pizzella ◽  
L. Coccato ◽  
...  
Keyword(s):  
Black Holes ◽  
Emission Line ◽  
Supermassive Black Holes ◽  
Archival Data ◽  
Early Type ◽  
Preliminary Results ◽  
Upper Limits ◽  
Nearby Galaxies ◽  
Line Widths

AbstractThe growth of supermassive black holes (SMBHs) appears to be closely linked with the formation of spheroids. There is a pressing need to acquire better statistics on SMBH masses, since the existing samples are preferentially weighted toward early-type galaxies with very massive SMBHs. With this motivation we started a project aimed at measuring upper limits on the mass of the SMBHs that can be present in the center of all the nearby galaxies (D < 100 Mpc) for which STIS/G750M spectra are available in the HST archive. These upper limits will be derived by modeling the central emission-line widths ([N II] λλ6548, 6583, Hα and [S II] λλ6716, 6731) observed over an aperture of ~01 (R < 50 pc). Here we present our preliminary results for a subsample of 76 bulges.

Nuclear magnetic resonance spectroscopy of denatured proteins

1969 ◽  
Vol 22 (5) ◽  
pp. 1083 ◽  
Author(s):  
JH Bradbury ◽  
NLR King
Keyword(s):  
Molecular Weight ◽  
Magnetic Resonance ◽  
Magnetic Resonance Spectroscopy ◽  
Trifluoroacetic Acid ◽  
Guanidine Hydrochloride ◽  
Dichloroacetic Acid ◽  
Random Coil ◽  
Resonance Spectroscopy ◽  
Line Broadening ◽  
Line Widths

The proton magnetic resonance spectroscopy of 11 proteins (molecular weight range 5700-650000) has been investigated in five denaturing solvents, viz., trifluoroacetic acid-d, formic acid, dichloroacetic acid, 6M guanidine hydrochloride in D2O, and 8M urea in D2O. The chemical shifts, line-widths, and intensities of the resonances have been measured of the histidine C2 protons, the methionine SCH3 protons and methyl protons of leucine, isoleucine, and valine, the aromatic protons, and the α-CH protons. ��� It is found that, with some exceptions delineated below, the line- widths of the methyl resonances are constant for a particular solvent, independent of the molecular weight of the protein. This indicates that, in general, the proteins behave as random coil structures in these solvents, which confirms the conclusion reached by Tanford and co-workers1-4 for 6M guanidine hydrochloride. ��� However, methyl line broadening occurs in dichloroacetic acid for catalase and fibrinogen, in guanidine hydrochloride for insulin, and in urea for insulin and lysozyme. Furthermore, the C 2 histidine resonance is absent in dichloroacetic acid solutions of thyroglobulin, catalase, and fibrinogen; the SCH3 resonance is absent in myoglobin in trifluoroacetic acid-d and occurs as a doublet for trypsin in guanidine hydrochloride and in urea. A general line broadening of resonances indicates association and/or incomplete unfolding of molecules, whereas perturbations of only one particular resonance, as in the cases detailed above, are probably due to intramolecular non-covalent interactions which involve the perturbed group and another unspecified group in the protein. ��

scholarly journals Line Broadening Data: Stark Broadening of Ca II Sc III And Ti IV Lines

1993 ◽  
Vol 137 ◽  
pp. 260-262
Author(s):  
Milan S. Dimitrijević ◽  
Sylvie Sahal-Bréchot
Keyword(s):  
Stark Broadening ◽  
Isoelectronic Sequence ◽  
Line Broadening ◽  
Proton Impact ◽  
Line Widths ◽  
And Shifts

AbstractElectron– and proton–impact line widths and shifts for important Ca II, Sc III and Ti IV lines, have been calculated using the semiclassical–perturbation formalism. The obtained results were used to investigate the behaviour of Stark broadening parameters within the K I isoelectronic sequence.

K emission-line widths and the solar chromosphere

Solar Physics ◽  
1971 ◽  
Vol 17 (2) ◽  
pp. 316-330 ◽  
Author(s):  
M. K. V. Bappu ◽  
K. R. Sivaraman
Keyword(s):  
Emission Line ◽  
Solar Chromosphere ◽  
Line Widths
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