scholarly journals The crystallographic and optical properties of iodo-succinimide

During the progress of the X-ray research on this substance by Miss Yardley, the results of which are embodied in the preceding communication, the need for a thorough reinvestigation of the crystallographic and especially the optical properties of the substance, was made very clear. The difficulty as regards the optical constants was that of preparing the properly orientated and absolutely truly plane-surfaced section-plates and 60°-prisms of this relatively soft and fragile substance, and after many attempts of a really heroic nature Miss Yardley appealed to the author, who was only too pleased to bring into service his cutting-and-grinding goniometer, with which the necessary plates and prisms were successfully prepared. The author, however, becoming very interested in the substance, has carried out also a complete goniometrical remeasurement, in the light of the new and correct setting which Miss Yardley has indicated, and a determination of the density of the crystals, so that with the optical data, now given for the first time, a revised and much more complete crystallographic description is herewith given. It agrees in every respect with the conclusions of Miss Yardley, as described in the immediately preceding communication. The only real difficulty met with, which renders the substance unusual to deal with, is the fact that no cementing material has been found which is without action on iodo-succinimide. For instance, Canada balsam and its solution in benzene (a hydrocarbon which, very fortunately, does not act on iodo-succinimide) or turpentine at once turn deep brown to black when used to cement section-plates to cover-glasses or to the little circular plates of parallel glass which the author uses in the preparation of the second surface. So that, after the first surface of a section-plate has been ground, the crystal being held as usual on the crystal holder by opticians’ hard wax, any action not mattering much here, the usual process—of cementing the crystal by this first surface on to one of the little glass discs, fitting the latter into the receptacle for it in the parallel-plate, preparing fitting of the cutting-and-grinding goniometer, and grinding the second surface without further trouble and thus making a plate as thin as may be desired—cannot be employed with iodo-succinimide. To prepare the second surface the crystal must be reset goniometrically, while held in a grip-holder instead of the usual holder carrying opticians’ wax, and then ground and polished with great care to avoid slipping in the gripper. As the substance is soft and friable this is rather a nuisance, especially, moreover, as it was desirable to be able to obtain section-plates of considerable tenuity for the purposes of Laue photographic X-ray analysis, as well as very thick ones for the study of possible optical activity. Happily, however, all these unusual difficulties were eventually overcome, and the desired results obtained.

2020 ◽  
Vol 34 (26) ◽  
pp. 2050229
Author(s):  
Fatemeh Zahraei ◽  
Ferydon Babaei ◽  
Ali Ehsani

Graphene-Nickel Oxide (G-NiO) nanocomposites with different morphologies, such as nanowires (NWs), nanorods (NRs) and nanoparticles (NPs), are synthesized by a combination of liquid-phase exfoliation (LPE) and hydrothermal methods. The synthesis of Graphene, morphology of Nickel Oxide (NiO) thin films and concentration of elements are analyzed using Raman Spectroscopy, Field Emission Scanning Electron Microscopy (FESEM) and Energy-dispersive X-ray spectroscopy (EDS), respectively. Furthermore, the capacitive behavior of nanocomposites is investigated using the Cyclic Voltammetry (CV). The optical properties of samples are extracted from measured absorbance spectra. Our results show that G-NiO NWs with the longest length have the largest specific capacitance (SC). In addition, optical data revealed that the adding Graphene to NiO thin films decreased the optical bandgap as well as the optical conductivity of nanocomposites increased with photon energy due to excitation electrons.


2018 ◽  
Vol 4 (10) ◽  
pp. eaat7259 ◽  
Author(s):  
Nan Yan ◽  
Nan Xia ◽  
Lingwen Liao ◽  
Min Zhu ◽  
Fengming Jin ◽  
...  

The transition from nanocluster to nanocrystal is a central issue in nanoscience. The atomic structure determination of metal nanoparticles in the transition size range is challenging and particularly important in understanding the quantum size effect at the atomic level. On the basis of the rationale that the intra- and interparticle weak interactions play critical roles in growing high-quality single crystals of metal nanoparticles, we have reproducibly obtained ideal crystals of Au144(SR)60 and successfully solved its structure by x-ray crystallography (XRC); this structure was theoretically predicted a decade ago and has long been pursued experimentally but without success until now. Here, XRC reveals an interesting Au12 hollow icosahedron in thiolated gold nanoclusters for the first time. The Au–Au bond length, close to that of bulk gold, shows better thermal extensibility than the other Au–Au bond lengths in Au144(SR)60, providing an atomic-level perspective because metal generally shows better thermal extensibility than nonmetal materials. Thus, our work not only reveals the mysterious, long experimentally pursued structure of a transition-sized nanoparticle but also has important implications for the growth of high-quality, single-crystal nanoparticles, as well as for the understanding of the thermal extensibility of metals from the perspective of chemical bonding.


2012 ◽  
Vol 32 (8) ◽  
pp. 0831001
Author(s):  
贾红宝 Jia Hongbao ◽  
孙菁华 Sun Jinghua ◽  
徐耀 Xu Yao ◽  
吴东 Wu Dong ◽  
吕海兵 Lü Haibing ◽  
...  

2019 ◽  
Vol 486 (4) ◽  
pp. 4863-4879 ◽  
Author(s):  
Ali Takey ◽  
Florence Durret ◽  
Isabel Márquez ◽  
Amael Ellien ◽  
Mona Molham ◽  
...  

ABSTRACT We present X-ray and optical properties of the optically confirmed galaxy cluster sample from the 3XMM/SDSS Stripe 82 cluster survey. The sample includes 54 galaxy clusters in the redshift range of 0.05–1.2, with a median redshift of 0.36. We first present the X-ray temperature and luminosity measurements that are used to investigate the X-ray luminosity–temperature relation. The slope and intercept of the relation are consistent with those published in the literature. Then, we investigate the optical properties of the cluster galaxies including their morphological analysis and the galaxy luminosity functions (GLFs). The morphological content of cluster galaxies is investigated as a function of cluster mass and distance from the cluster centre. No strong variation of the fraction of early- and late-type galaxies with cluster mass is observed. The fraction of early-type galaxies as a function of cluster radius varies as expected. The individual GLFs of red sequence galaxies were studied in the five ugriz bands for 48 clusters. The GLFs were then stacked in three mass bins and two redshift bins. Twenty clusters of the present sample are studied for the first time in X-rays, and all are studied for the first time in the optical range. Altogether, our sample appears to have X-ray and optical properties typical of ‘average’ cluster properties.


1984 ◽  
Vol 48 (348) ◽  
pp. 389-396 ◽  
Author(s):  
F. Moore ◽  
R. A. Howie

Abstract The result of electron probe microanalyses, along with X-ray and optical data obtained for tin sulphides from two different localities in south-west England indicate that the mineral hitherto described from St Michael’s Mount as stannite is in fact kesterite, Cu2(Fe0.23Zn0.77)SnS4. The yellow ‘stannite’ reported from this locality proved to be stannoidite, Cu8(Fe2.39 Zn0.61)SnS2S12. Kesterite, Cu2(Fe0.09Zn0.90SnS4, and zincian stannite, Cu2(Fe0.63Zn0.38)SnS4, are also reported from Cligga Head. It is suggested that a more cautious approach should be taken in identifying these tin sulphides solely on their optical properties.


2019 ◽  
Vol 627 ◽  
pp. A2
Author(s):  
Gregor Rauw ◽  
Yaël Nazé ◽  
Fran Campos

Aims. The Cyg OB2 #5 system is thought to consist of a short-period (6.6 d) eclipsing massive binary orbited by an OB-star with a period of ~6.7 yr; these stars in turn are orbited by a distant early B-star with a period of thousands of years. However, while the inner binary has been studied many times, information is missing on the other stars, in particular the third star whose presence was indirectly postulated from recurrent modulations in the radio domain. Besides, to this date, the X-ray light curve could not be fully interpreted, for example in the framework of colliding-wind emission linked to one of the systems. Methods. We obtained new optical and X-ray observations of Cyg OB2 #5, which we combined to archival data. We performed a thorough and homogeneous investigation of all available data, notably revisiting the times of primary minimum in photometry. Results. In the X-ray domain, XMM-Newton provides scattered exposures over ~5000 d whilst Swift provides a nearly continuous monitoring for the last couple of years. Although the X-ray light curve reveals clear variability, no significant period can be found hence the high-energy emission cannot be explained solely in terms of colliding winds varying along either the short or intermediate orbits. The optical data reveal for the first time clear signs of reflex motion. The photometry indicates the presence of a 2366 d (i.e. 6.5 yr) period while the associated radial velocity changes are detected at the 3σ level in the systemic velocity of the He II λ 4686 emission line. With the revised period, the radio light curve is interpreted consistently in terms of a wind interaction between the inner binary and the tertiary star. From these optical and radio data, we derive constraints on the physical properties of the tertiary star and its orbit.


1989 ◽  
Vol 42 (7) ◽  
pp. 1103 ◽  
Author(s):  
CO Miles ◽  
L Main ◽  
BK Nicholson

Two improved general routes to 2′,6′-dihydroxychalcones are described in which the final step is protective-group removal from O 2′ under mild acid conditions. The first involves base-catalysed condensation of benzaldehydes with 2′-hydroxy-6′-tetrahydropyran-2-yloxyacetophenone, the second ring-opening of 5-hydroxyflavanones with 1,8-diazabicyclo[5.4.0]undec-7-ene in the presence of a trialkylchlorosilane to trap out the chalcone as a bis silyl ether. Chalcones prepared by the first route are 2',6'-dihydroxychalcone (1), and its 4-methoxy (2), 3,4-dimethoxy (3), 3,4,5-trimethoxy (4), and 2,4,6-trimethoxy (5) derivatives. The 4-chloro derivative (6) and the chalcone from hesperetin are prepared by the second method. .The X-ray crystal structure of 2',6'-dihydroxy-2,4,6-trimethoxychalcone (5), the first for a 2',6′-dihydroxychalcone, is reported, the hydrogen involved in intramolecular hydrogen-bonding between the carbonyl and phenolic oxygens being located for the first time for any 2'-hydroxychalcone derivative. The O 6' involved in the intramolecular hydrogen-bonding is also hydrogen-bonded intermolecularly to the hydrogen of the other (2'-)hydroxy group of a neighbouring molecule in the lattice. 13C n.m.r. data are the first reported for a series of 2',6'-dihydroxychalcones.


Author(s):  
A. M. Afanas'ev ◽  
R. M. Imamov ◽  
E. Kh. Mukhamedzhanov ◽  
A. N. Chuzo

A simple relation has been established between the Fourier component of the probability density P(z) of photoelectron emission from different depths of a crystal and the angular dependence of the emission of photoelectrons formed in inclined X-ray Laue diffraction, which for the first time permitted the use of a direct method for the reconstruction of the P(z) function. Accurate measurements of the angular dependence of photoelectron emission were carried out on a silicon single crystal with diffraction of Cu Kα radiation for different energy ranges. Photoelectrons were recorded by a proportional gas counter specially designed for the energy analysis of photoelectrons under inclined Laue diffraction conditions. The laws predicted by the theory have been fully confirmed, and the corresponding P(z) functions have been obtained.


Soil Research ◽  
1989 ◽  
Vol 27 (2) ◽  
pp. 275 ◽  
Author(s):  
CW Ross ◽  
G Mew ◽  
CW Childs

Deeply cemented quartzofeldspathic and ilmenitic sands occur on and beneath uplifted late Quaternary marine terrace surfaces over wide areas south of Westport on the west coast of the South Island. These terraces are weakly dissected, but are mainly flat to rolling. Rainfall averages about 3000 mm per year. Present vegetation consists of pasture, scrub and rush/fern associations which have replaced podocarp forest. Cementation of sands has resulted in impeded drainage, limited rooting volumes for trees and crops, and other limitations to land development. Two soil series, Charleston and Marris, were studied, as they were distinguished by having different forms of cementation in the field. Techniques used to investigate cementation included the determination of Fe, Al and Si contents by extraction with standard chemical reagents, X-ray diffractometry to identify minerals of short-range order, SEM to examine microstructures, EDAX to determine elemental composition, and heating in an induction furnace to evaluate C content. Two apparent causes of cementation were identified, namely ferrihydrite in the Charleston soil, and allophane with humus-aluminium complexes in the Marris soil. Microstructures of sand cemented by these materials were clearly different. In the Charleston soil, iron-rich material coating sand grains and bridging between them is smooth and gel-like and has a fine globular appearance under high magnification. In the Marris soil, the cementing material has a rough-textured fibrous appearance. The contrasts in types of cementing agents are thought to be related to firstly, differences in physiography at time of formation and secondly, different drainage conditions related to topographic position.


2020 ◽  
Vol 642 ◽  
pp. L3
Author(s):  
X. Zhang ◽  
A. Simionescu ◽  
J. S. Kaastra ◽  
H. Akamatsu ◽  
D. N. Hoang ◽  
...  

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV Heα X-ray emission line is clearly visible in the 25 ks observation, allowing a precise determination of the redshift of the cluster as z = 0.180 ± 0.006. We measure kT500 = 8.3  ±  0.4 keV and estimate M500 = (1.06 ± 0.11) × 1015 M⊙ based on existing scaling relations. Correcting both the radio and X-ray luminosities with the revised redshift reported here, which is much larger than previously inferred based on sparse optical data, this object is no longer an X-ray underluminous outlier in the LX − Pradio scaling relation. The new redshift also means that, in terms of physical scale, ClG 0217+70 hosts one of the largest radio halos and one of the largest radio relics known to date. Most of the relic candidates lie in projection beyond r200. The X-ray morphological parameters suggest that the intracluster medium is still dynamically disturbed. Two X-ray surface brightness discontinuities are confirmed in the northern and southern parts of the cluster, with density jumps of 1.40 ± 0.16 and 3.0 ± 0.6, respectively. We also find a 700 × 200 kpc X-ray faint channel in the western part of the cluster, which may correspond to compressed heated gas or increased non-thermal pressure due to turbulence or magnetic fields.


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