scholarly journals HTLV-1, the Other Pathogenic Yet Neglected Human Retrovirus: From Transmission to Therapeutic Treatment

Viruses ◽  
2017 ◽  
Vol 10 (1) ◽  
pp. 1 ◽  
Author(s):  
Nicolas Futsch ◽  
Renaud Mahieux ◽  
Hélène Dutartre
1976 ◽  
Vol 62 (4) ◽  
pp. 365-372 ◽  
Author(s):  
Sante Basso Ricci ◽  
Vittorio Ventafridda ◽  
Rita Zanolla ◽  
Lia Cassani ◽  
Roberto Spreafico

A study was carried out on a series of 25 patients who were operated on for breast cancer and who submitted to postoperative radiotherapy, in which lesions of the brachial nervous plexus from ionizing radiations were obtained. In almost all the cases, 24 out of 25, various symptoms such as paresthesiae, pain, and motorial disturbances, were observed even one year after the completion of the treatment. Motorial troubles, which in 13 cases were not detected at the moment of the diagnosis of the other lesions, always occurred later. Etiopathogenesis and diagnosis of these lesions have been considered, as well as the possibility of lowering the incidence of such troubles. The conclusion can be drawn that useful results can be obtained, to a certain extent, only if therapeutic treatment is performed early: in most cases, however, the lesions showed a progressive evolution.


2020 ◽  
Vol 8 (8) ◽  
pp. 4050-4057
Author(s):  
Monika Gupta ◽  
Shakshi Kangotra

Vatarakta is a Vatavyadhi Prabheda. The illness is considered to be the finest illustration of an Avarana Vyadhi, as an opening from the etiopathogenesis to the complications, the illness follows the characteristic presentation of Avarana. Compared with the other Vatavyadhi, Vatarakta possesses a special place in the literature, due to its high prevalence in the society, increased incidence as age advances, stepwise succes-sion, and so on. From the overall view of the etiology, it is obvious and unambiguous that the precise etio-logical factors of Vata Dosha as well as Rakta Dhatu are accountable for the causation of illness. The ety-mology and symptomatology of Vatarakta is very much similar to that of Hyperuricemia. Whatever be the grounds, an obstruction in the path of Rakta Dhatu is the core pathology of the disease. In this single group study, 30 patients diagnosed of Vatarakta were selected randomly for an open trial of Anubhoot Yoga for a period of 60 days with life style modifications to provide safe ,effective and conservative treatment for Vatarakta w.s.r.to hyperuricemia In the present study as per the clinical data, Anubhoot yoga is the reliable therapeutic treatment of Vatarakta.


2016 ◽  
Vol 16 (11) ◽  
pp. 1205-1206 ◽  
Author(s):  
Sarah Mollenkopf ◽  
Edward L Murphy
Keyword(s):  

1988 ◽  
Vol 62 (03) ◽  
pp. 411-419 ◽  
Author(s):  
Colin W. Stearn

Stromatoporoids are the principal framebuilding organisms in the patch reef that is part of the reservoir of the Normandville field. The reef is 10 m thick and 1.5 km2in area and demonstrates that stromatoporoids retained their ability to build reefal edifices into Famennian time despite the biotic crisis at the close of Frasnian time. The fauna is dominated by labechiids but includes three non-labechiid species. The most abundant species isStylostroma sinense(Dong) butLabechia palliseriStearn is also common. Both these species are highly variable and are described in terms of multiple phases that occur in a single skeleton. The other species described areClathrostromacf.C. jukkenseYavorsky,Gerronostromasp. (a columnar species), andStromatoporasp. The fauna belongs in Famennian/Strunian assemblage 2 as defined by Stearn et al. (1988).


1967 ◽  
Vol 28 ◽  
pp. 207-244
Author(s):  
R. P. Kraft

(Ed. note:Encouraged by the success of the more informal approach in Christy's presentation, we tried an even more extreme experiment in this session, I-D. In essence, Kraft held the floor continuously all morning, and for the hour and a half afternoon session, serving as a combined Summary-Introductory speaker and a marathon-moderator of a running discussion on the line spectrum of cepheids. There was almost continuous interruption of his presentation; and most points raised from the floor were followed through in detail, no matter how digressive to the main presentation. This approach turned out to be much too extreme. It is wearing on the speaker, and the other members of the symposium feel more like an audience and less like participants in a dissective discussion. Because Kraft presented a compendious collection of empirical information, and, based on it, an exceedingly novel series of suggestions on the cepheid problem, these defects were probably aggravated by the first and alleviated by the second. I am much indebted to Kraft for working with me on a preliminary editing, to try to delete the side-excursions and to retain coherence about the main points. As usual, however, all responsibility for defects in final editing is wholly my own.)


1967 ◽  
Vol 28 ◽  
pp. 177-206
Author(s):  
J. B. Oke ◽  
C. A. Whitney

Pecker:The topic to be considered today is the continuous spectrum of certain stars, whose variability we attribute to a pulsation of some part of their structure. Obviously, this continuous spectrum provides a test of the pulsation theory to the extent that the continuum is completely and accurately observed and that we can analyse it to infer the structure of the star producing it. The continuum is one of the two possible spectral observations; the other is the line spectrum. It is obvious that from studies of the continuum alone, we obtain no direct information on the velocity fields in the star. We obtain information only on the thermodynamic structure of the photospheric layers of these stars–the photospheric layers being defined as those from which the observed continuum directly arises. So the problems arising in a study of the continuum are of two general kinds: completeness of observation, and adequacy of diagnostic interpretation. I will make a few comments on these, then turn the meeting over to Oke and Whitney.


1966 ◽  
Vol 24 ◽  
pp. 337
Author(s):  
W. Iwanowska

A new 24-inch/36-inch//3 Schmidt telescope, made by C. Zeiss, Jena, has been installed since 30 August 1962, at the N. Copernicus University Observatory in Toruń. It is equipped with two objective prisms, used separately, one of crown the other of flint glass, each of 5° refracting angle, giving dispersions of 560Å/mm and 250Å/ mm respectively.


2020 ◽  
Vol 43 ◽  
Author(s):  
Philip Pettit

Abstract Michael Tomasello explains the human sense of obligation by the role it plays in negotiating practices of acting jointly and the commitments they underwrite. He draws in his work on two models of joint action, one from Michael Bratman, the other from Margaret Gilbert. But Bratman's makes the explanation too difficult to succeed, and Gilbert's makes it too easy.


1999 ◽  
Vol 173 ◽  
pp. 249-254
Author(s):  
A.M. Silva ◽  
R.D. Miró

AbstractWe have developed a model for theH2OandOHevolution in a comet outburst, assuming that together with the gas, a distribution of icy grains is ejected. With an initial mass of icy grains of 108kg released, theH2OandOHproductions are increased up to a factor two, and the growth curves change drastically in the first two days. The model is applied to eruptions detected in theOHradio monitorings and fits well with the slow variations in the flux. On the other hand, several events of short duration appear, consisting of a sudden rise ofOHflux, followed by a sudden decay on the second day. These apparent short bursts are frequently found as precursors of a more durable eruption. We suggest that both of them are part of a unique eruption, and that the sudden decay is due to collisions that de-excite theOHmaser, when it reaches the Cometopause region located at 1.35 × 105kmfrom the nucleus.


1975 ◽  
Vol 26 ◽  
pp. 395-407
Author(s):  
S. Henriksen

The first question to be answered, in seeking coordinate systems for geodynamics, is: what is geodynamics? The answer is, of course, that geodynamics is that part of geophysics which is concerned with movements of the Earth, as opposed to geostatics which is the physics of the stationary Earth. But as far as we know, there is no stationary Earth – epur sic monere. So geodynamics is actually coextensive with geophysics, and coordinate systems suitable for the one should be suitable for the other. At the present time, there are not many coordinate systems, if any, that can be identified with a static Earth. Certainly the only coordinate of aeronomic (atmospheric) interest is the height, and this is usually either as geodynamic height or as pressure. In oceanology, the most important coordinate is depth, and this, like heights in the atmosphere, is expressed as metric depth from mean sea level, as geodynamic depth, or as pressure. Only for the earth do we find “static” systems in use, ana even here there is real question as to whether the systems are dynamic or static. So it would seem that our answer to the question, of what kind, of coordinate systems are we seeking, must be that we are looking for the same systems as are used in geophysics, and these systems are dynamic in nature already – that is, their definition involvestime.


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