Exploring the impact of osteopathic treatment on cranial asymmetries associated with nonsynostotic plagiocephaly in infants

2011 ◽  
Vol 17 (4) ◽  
pp. 193-198 ◽  
Author(s):  
Sylvie Lessard ◽  
Isabelle Gagnon ◽  
Nathalie Trottier
Keyword(s):  
Osteopathic Treatment ◽  
Nonsynostotic Plagiocephaly ◽  
The Impact

Effects of a General Osteopathic treatment on asthmatic children

2020 ◽  
pp. 137-145
Author(s):  
B. Ernoult ◽  
H. Job
Keyword(s):  
Asthmatic Child ◽  
Daily Basis ◽  
Short Term ◽  
Asthmatic Children ◽  
Lung Capacity ◽  
Before And After ◽  
Osteopathic Treatment ◽  
Residual Capacity ◽  
Term Basis ◽  
The Impact

Aim. Up to 10 % of population suffer from asthma. Asthma often means managing a treatment with limited action on a daily basis. The study aim was to assess the impact of a General Osteopathic treatment (GOT) on the respiratory function in asthmatic children.Method. 15 asthmatic subjects, aged 4 to 15, diagnosed by an allergologist, received one GOT session. Objective results were obtained through a bodyplethysmography measure before and after treatment. Variables observed were: Tiffeneau′s coefficient, mean expiratory fl ow from small bronchial tubes, bronchial resistances and residual capacity.Results. Comparison between result before and after treatment showed a significant improvement of all measures after the GOT.Conclusions. On a short term basis, a session of GOT allows to asthmatic child to improve its lung capacity. Including Osteopathy in the pluridisciplinary care of asthmatic children appears to be relevant. 

Secondary effects and quality of life with chemotherapy: assessing the impact of an osteopathic treatment (multicentric randomized clinical trial)

2020 ◽  
pp. 174-185
Author(s):  
N. Favier ◽  
A. G. Guinet ◽  
M. Nageleisen ◽  
B. Ceccaldi ◽  
E. Pujade-Lauraine ◽  
...  
Keyword(s):  
Quality Of Life ◽  
Shortness Of Breath ◽  
Secondary Effects ◽  
Treatment Control ◽  
Fully Integrated ◽  
Treatment Stage ◽  
Osteopathic Treatment ◽  
And Control ◽  
The Impact

The goal of research. The purpose of this work was to assess the effectiveness of osteopathic treatment aimed to improve the quality of life of patients receiving chemotherapy.Materials and methods. The study was conducted by four osteopaths at the oncology departments of four hospitals in Paris region. Patients were randomly divided into two groups. Patients of the first group received osteopathic treatment first, and then a placebo was used. Patients of the second group received the placebo first and then osteopathic treatment. We used a cross-protocol during two consecutive courses of treatment: each patient served as his or her own control. During the treatment stage osteopathic therapy was used; when the patient was control, the osteopathic treatment was imitated. A modified QLQ-C30 questionnaire was used as an evaluation criterion. It was fi lled in three times: before osteopathic treatment (control), after real treatment (treatment) and after simulated treatment (placebo).Results. The study involved 40 patients — 27 women and 13 men. The differences between the treatment and control stages were very highly significant for such criteria as nausea, vomiting and shortness of breath, highly significant for such criteria as fatigue, and significant for such criteria as pain and sleep disturbance. Efficiency was statistically higher compared with placebo for all of these criteria. No differences were found associated with the sequence of real or simulated treatment, as well as with the variability of osteopaths in different centers.Conclusion. The results of this study indicate that osteopathy is a clinically effective method of correction of side effects in patients receiving chemotherapy. These results are interesting enough to suggest that the presence of osteopaths at oncology departments may be useful for cancer patients. Subsequent studies should confirm these results and quantify the effectiveness of osteopathic correction, so that it could be fully integrated into the classical treatment.

scholarly journals An evaluation of osteopathic treatment on psychological outcomes with patients suffering from chronic pain: A prospective observational cohort study collected through a health and well-being academy

2018 ◽  
Vol 5 (1) ◽  
pp. 205510291877468 ◽  
Author(s):  
Darren J Edwards ◽  
Craig Toutt
Keyword(s):  
Mental Health ◽  
Chronic Pain ◽  
Controlled Trial ◽  
Well Being ◽  
Fear Avoidance ◽  
Psychological Outcome ◽  
Osteopathic Treatment ◽  
Randomised Controlled ◽  
Anxiety Depression ◽  
The Impact

Co-morbid mental health conditions such as anxiety, depression and fear avoidance are often associated with chronic pain. This novel study aimed to explore the impact of osteopathic treatment on several psychological outcome measures relating to anxiety, depression, mental health and fear avoidance for a chronic pain population receiving osteopathic treatment over a 2-week period. The findings show that there were significant reductions in anxiety, pain, mental health dysfunction and improvements in self-care. These results are promising, and it is suggested that now a full-scale randomised controlled trial should be conducted.

Formation of Lunar Craters and Bright Rays as a Result of Meteorite Impacts

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten
Keyword(s):  
Explosive Charge ◽  
The Moon ◽  
Meteorite Impacts ◽  
The Earth ◽  
Lunar Craters ◽  
The Impact

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.

The Geosciences Applied to Lunar Exploration

1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green
Keyword(s):  
Lunar Surface ◽  
Probable Mechanism ◽  
Point Of View ◽  
Lunar Exploration ◽  
Geological Model ◽  
Apply Geophysics ◽  
Surface Features ◽  
The Impact

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.

Asteroid and Comet Impact Speeds upon Mars: Significance for Panspermia and the Supply of Organics

1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel
Keyword(s):  
Probability Distributions ◽  
Regions Of Interest ◽  
Significant Fraction ◽  
Organic Chemicals ◽  
Impact Speed ◽  
The Mean ◽  
The Impact

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.

Organic Syntheses During the Impact of a Comet with a Gaseous Planet

1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini
Keyword(s):  
Polymeric Material ◽  
Molecular Form ◽  
Parent Compound ◽  
Blue Filter ◽  
Organic Syntheses ◽  
The Impact

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.

Hydrogen Cyanide Polymers from the Impact of Comet P/Shoemaker-Levy 9 on Jupiter

1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman
Keyword(s):  
Amino Acids ◽  
Solar System ◽  
Hydrogen Cyanide ◽  
Nitrogen Heterocycles ◽  
Laboratory Studies ◽  
Heterogeneous Solids ◽  
The Many ◽  
Comet Halley ◽  
The Impact ◽  
By Products

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.

Unusual Microstructure in Shock-Compacted Graphite

1970 ◽  
Vol 28 ◽  
pp. 474-475
Author(s):  
Lucien F. Trueb
Keyword(s):  
Mechanical Characteristic ◽  
Compression Wave ◽  
Gray Zone ◽  
Flyer Plate ◽  
Compacted Graphite ◽  
The Impact

Crushed and statically compressed Madagascar graphite that was explosively shocked at 425 kb by means of a planar flyer-plate is characterized by a black zone extending for 2 to 3 nun below the impact plane of the driver. Beyond this point, the material assumes the normal gray color of graphite. The thickness of the black zone is identical with the distance taken by the relaxation wave to overtake the compression wave.The main mechanical characteristic of the black material is its great hardness; steel scalpels and razor blades are readily blunted during attempts to cut it. An average microhardness value of 95-3 DPHN was obtained with a 10 kg load. This figure is a minimum because the indentations were usually cracked; 14.8 DPHN was measured in the gray zone.

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