scholarly journals X‐Ray Spectroscopic Observations of EX Hydrae and Mass Determination of the White Dwarf

1997 ◽  
Vol 474 (2) ◽  
pp. 774-781 ◽  
Author(s):  
Ryuichi Fujimoto ◽  
Manabu Ishida
2019 ◽  
Vol 1354 ◽  
pp. 012014
Author(s):  
H Wulandari ◽  
A H Fikri ◽  
K Vierdayanti ◽  
A N I Putri ◽  
D G Ramadhan

1972 ◽  
Vol 37 (1) ◽  
pp. 115-124
Author(s):  
V.W. Steward ◽  
S. Rudofsky

2020 ◽  
Vol 9 ◽  
pp. 308
Author(s):  
D. F. Anagnostopoulos, et al.

X-ray transitions in pionic nitrogen were measured using a curved crystal spectrometer. From the transition energy, calibrated with the help of the copper Ka1,2 electronic transition, a value for the charged pion mass of (139.57071± 0.00053) MeV/c2 was deduced. In order to reduce the uncertainty of the charged pion mass in the level of 1 ppm, we propose the determination of pionic transition energy based on the more precisely known energies and line shapes of muonic transitions.


2015 ◽  
Vol 1085 ◽  
pp. 455-459 ◽  
Author(s):  
Sergei P. Osipov ◽  
Vasilii A. Klimenov ◽  
Oleg S. Osipov ◽  
Vil'dan D. Samigullin ◽  
Aleksandr M. Shtein

The paper presents foundations of the algorithm of processing primary radiographic images of large-size cargoes that allows determination of their masses. Two possible approaches to form definite algorithm of processing radiographic information were analyzed. The choice of the approaches depends on the completeness of information about the test object. The first approach to design mass determination algorithm is connected with inspecting industrial products. Industrial inspecting products are characterized by a completeness of information about the material, its structure, the geometry. The information augmented by selecting maximum X-ray energy and calibrating by test object allows determination the mass of inspecting object by the only radiographic image with high precision. The second approach is caused by indeterminacy and incomplete information about inspecting object. This case is typical for problems of cargo inspection. Corresponding algorithm modification is based on using dual-energy X-ray imaging that allows determination of the effective atomic number of test object and provision of the required precision of mass estimation.


2004 ◽  
Author(s):  
Chithra Karunakaran ◽  
Digvir S. Jayas ◽  
Noel. D. G. White

1983 ◽  
Vol 72 ◽  
pp. 25-28 ◽  
Author(s):  
D. Crampton ◽  
A.P. Cowley ◽  
J.B. Hutchings

ABSTRACTSpectroscopic observations of two very different objects are discussed: the first, SS433, is a wery massive binary system probably containing an unseen 0 or WR star and a black hole surrounded by a luminous precessing accretion disk (from which emanate spectacular relativistic jets); the second, GK Per, is a classical old nova consisting of a slightly evolved K2 star and an unseen white dwarf companion surrounded by an accretion disk which is less luminous than the K2 star.


Author(s):  
H.J. Dudek

The chemical inhomogenities in modern materials such as fibers, phases and inclusions, often have diameters in the region of one micrometer. Using electron microbeam analysis for the determination of the element concentrations one has to know the smallest possible diameter of such regions for a given accuracy of the quantitative analysis.In th is paper the correction procedure for the quantitative electron microbeam analysis is extended to a spacial problem to determine the smallest possible measurements of a cylindrical particle P of high D (depth resolution) and diameter L (lateral resolution) embeded in a matrix M and which has to be analysed quantitative with the accuracy q. The mathematical accounts lead to the following form of the characteristic x-ray intens ity of the element i of a particle P embeded in the matrix M in relation to the intensity of a standard S


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