Study of equilibrium and non-equilibrium intergranular segregations of sulphur in nickel by high resolution microprints and electrochemical testing

1982 ◽  
Vol 17 (2) ◽  
pp. 387-396 ◽  
Author(s):  
J. Barbier-Vitart ◽  
G. Saindrenan ◽  
A. Larere ◽  
C. Roques-Carmes
Keyword(s):  
High Resolution ◽  
Electrochemical Testing ◽  
Non Equilibrium

scholarly journals Predicting the stellar and non-equilibrium dust emission spectra of high-resolution simulated galaxies with dart-ray

2015 ◽  
Vol 449 (1) ◽  
pp. 243-267 ◽  
Author(s):  
Giovanni Natale ◽  
Cristina C. Popescu ◽  
Richard. J. Tuffs ◽  
Victor P. Debattista ◽  
Jörg Fischera ◽  
...  
Keyword(s):  
High Resolution ◽  
Dust Emission ◽  
Emission Spectra ◽  
Non Equilibrium

scholarly journals Non-Equilibrium Ionization in Puppis A

1983 ◽  
Vol 101 ◽  
pp. 245-252
Author(s):  
P. F. Winkler ◽  
C. R. Canizares ◽  
B. C. Bromley
Keyword(s):  
High Resolution ◽  
Spectroscopic Data ◽  
Supernova Remnant ◽  
Optical Data ◽  
Equilibrium Conditions ◽  
X Ray ◽  
Flux Measurements ◽  
Far From Equilibrium ◽  
Einstein Observatory ◽  
Non Equilibrium

High resolution X-ray spectroscopy of the brightest knot of emission in the Puppis A supernova remnant shows that it is made up of ionizing plasma, far from equilibrium. Flux measurements in several X-ray lines enable us to determine the non-equilibrium conditions: electron temperature, ion populations, and time since the knot was heated by the supernova shock. Imaging and spectroscopic data from the Einstein Observatory together suggest that this knot is a cloud of density about 10 cm−3 which has recently been shocked to a temperature 7 × 106 K. Radio and optical data on the region appear consistent with this picture.

scholarly journals A Comparison of Three Regions of Puppis A

1990 ◽  
Vol 115 ◽  
pp. 172-175
Author(s):  
K.F. Fischbach ◽  
L.M. Bateman ◽  
C.R. Canizares ◽  
T.H. Markert ◽  
P.J. Saez
Keyword(s):  
High Resolution ◽  
Shock Front ◽  
Electron Temperature ◽  
Plasma Diagnostics ◽  
Column Density ◽  
Equilibrium Analysis ◽  
Ionization Equilibrium ◽  
X Ray ◽  
Hydrogen Column Density ◽  
Non Equilibrium

AbstractHigh resolution X-ray spectral observations of Puppis A were performed with the FPCS on the Einstein Observatory at three regions of the remnant: the shock front, the bright eastern knot, and the interior. Plasma diagnostics of lines from OVII and OVIII constrain the values of electron temperature, ionization timescale, and hydrogen column density. We compare results of the diagnostics for these three regions. A non-equilibrium analysis of previously published fluxes of oxygen lines shows that the interior has not yet reached ionization equilibrium.

scholarly journals Equilibrium and Non-equilibrium Studies of Protein G using High-Resolution Optical Trapping Unveil Heterogeneous Unfolding Pathways

2018 ◽  
Vol 114 (3) ◽  
pp. 577a
Author(s):  
Yujie Chen ◽  
Dena Izadi ◽  
Miles L. Whitmore ◽  
Joseph D. Slivka ◽  
Lisa J. Lapidus ◽  
...  
Keyword(s):  
High Resolution ◽  
Optical Trapping ◽  
Protein G ◽  
Equilibrium Studies ◽  
Non Equilibrium
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