scholarly journals Intrinsic Variability of Wolf-Rayet Stars from an Observational Point of View

1991 ◽  
Vol 143 ◽  
pp. 109-124
Author(s):  
Anthony F. J. Moffat ◽  
Carmelle Robert

Evidence is mounting that the dominant random component of variability in single WR stars can be explained by one common phenomenon: stochastic formation, propagation and decay of density enhancements in the winds.

1986 ◽  
Vol 7 ◽  
pp. 237-246
Author(s):  
D. W. Kurtz

AbstractThe present state of our knowledge of non-radial oscillations in δ Scuti stars and Rapidly Oscillating Ap stars is discussed primarily from an observational point of view. For the δ Scuti stars the need for complete frequency solutions for multi-periodic non-radial oscillating stars is emphasized in order for stellar seismology of these stars to be possible. An introduction to the Rapidly Oscillating Ap stars is given along with reference to a more complete recent review of those stars.


2004 ◽  
Vol 118 (7) ◽  
pp. 487-488 ◽  
Author(s):  
S. Dietrich

Tinnitus, that is defined as ’ringing in the ear’, is and has probably always been a very common phenomenon in the health history of mankind. A variety of pathomechanisms for its onset has been proposed in the past and this trend sees no stopping. Precise pathomechanisms still remain unclear. From the historical point of view, tinnitus is a very interesting topic but there is a lack of scientific enquiries. As its earliest historic reference, the Papyrus Ebers is often cited. By reviewing the original source, however, it is very unlikely that this contains the earliest historic reference of tinnitus. It is rather likely indeed that tinnitus was a known symptom in the ancient Egypt but it has never been exclusively been written down. This article reviews data provided by this fascinating historical period on the questionable reference and highlights the impact of history on the modern status of tinnitus.


Author(s):  
Mikhail V. Vinichenko ◽  
Marina V. Rybakova ◽  
Galina Y. Nikiporets-Takigawa ◽  
Oхana L. Chulanova ◽  
Natalia V. Ljapunova

The article discusses the nature of the influence of artificial intelligence on the development of human potential from the point of view of the Orthodox clergy and their parishioners. Methodologically, surveys and statistics were used to find out the opinion of the study subjects. A common phenomenon in the study was a unique consolidated position of all categories of Orthodox respondents on the danger that artificial intelligence represents. Most Orthodox are concerned about the unpredictability of creating and using artificial intelligence, especially in a pandemic. The authors considered the position of clergy, parishioners with and without a church on the nature of artificial intelligence's influence on human potential, the threats and risks to humans that come from artificial intelligence. The main advantage of the work is the results obtained on the basis of the comparative analysis of the positions of different categories of orthodox respondents on the nature of the influence of artificial intelligence on the development of human potential. In conclusion, the results can be used to develop a categorical-conceptual apparatus, to systematize knowledge about the use of artificial intelligence in the social and spiritual spheres.


Author(s):  
Yoram Rubin

Stochastic hydrogeology is the study of hydrogeology using physical and probabilistic concepts. It is an applied science because it is oriented toward applications. Its goal is to develop tools for analyzing measurements and observations taken over a sample region in space, and extract information which can then be used for evaluating and modeling the properties of physical processes taking place in this domain, and make risk-qualified predictions of their outcome. By invoking probabilistic concepts to deal with problems of physics, stochastic hydrogeology joins a well-established tradition followed in mining (Matheron, 1965; David, 1977; Journel and Huijbregts, 1978), turbulence (Kolmogorov, 1941; Batchelor, 1949), acoustics (Tatarski, 1961), atmospheric science (Lumley and Panofsky, 1964), composite materials and electrical engineering (Beran, 1968; Batchelor, 1974), and of course statistical mechanics. Stochastic hydrogeology broadens the scope of the deterministic approach to hydrogeology by considering the last as an end member to a wide spectrum of states of knowledge, stretching from deterministic knowledge at one end all the way to maximum uncertainty at the other, with a continuum of states, representing varying degrees of uncertainty in the hydrogeological processes, in between. It provides a formalism for addressing this continuum of states systematically. The departure from the confines of determinism is an important and intuitively appealing paradigm shift, representing the maturing of hydrogeology from an exploratory into an applied discipline. Deterministic knowledge of a site’s hydrogeology is a state we rarely, if ever, find ourselves in, although from a fundamental point of view there is no inherent element of chance in the hydrogeological processes. For example, we know that mass conservation is a deterministic concept, and we are also confident that Darcy’s law works under conditions which are fairly well understood. However, the application of these principles involves a fair amount of conjecture and speculation, and hence when dealing with real-life applications, determinism exists only in the fact that uncertainty and ambiguity are unavoidable, and might as well be studied and understood. The other end of the spectrum is where uncertainty is the largest. Generally speaking, two types of uncertainty exist: intrinsic variability and epistemic uncertainty.


1988 ◽  
Vol 132 ◽  
pp. 485-492
Author(s):  
Pierre Magain

The possible existence of departures from LTE affecting the abundance analyses of halo dwarfs and subgiants is analysed from the observational point of view, and illustrated by the case of the intermediate halo subgiant HD 76932. High resolution and high S/N Reticon and CCD spectra have been obtained with the ESO Coude Echelle Spectrometer. A detailed model atmosphere analysis has been carried out, which reveals a number of inconsistencies. In particular, the iron abundance derived from the neutral lines shows a very clear excitation potential dependence. Similar effects appear for oxygen and calcium and, possibly, for magnesium, chromium and ionized iron. Some overionization also seems to be present in a number of elements. The impact of these effects on the derived abundances may be rather large (some 0.2 to 0.6 dex). In particular, doubts might be raised about the reality of the oxygen overabundance and the odd-even effect in Na, Mg and Al.


2020 ◽  
Vol 35 (02n03) ◽  
pp. 2040041
Author(s):  
J. C. Fabris ◽  
T. R. P. Caramês ◽  
A. Wojnar ◽  
H. E. S. Velten

Viscous properties are attributed to the dark sector of the Universe. They contribute to the accelerated expansion phase of the Universe and can alleviate existing tensions in the [Formula: see text]CDM model at small scales. We provide a short review of recent efforts on this topic. Different viscous models for the dark sector are analysed both from theoretical and observational point of view.


1974 ◽  
Vol 62 ◽  
pp. 239-246
Author(s):  
C. Allen ◽  
A. Poveda

To study the dynamical evolution of trapezia, the equations of motion of the member stars in 30 different trapezia were integrated numerically. It was found that two-thirds of the trapezia still remain as such after 106 yr. Thus, the dynamical ages of trapezia containing O-stars are only slightly shorter than their nuclear ages. The properties of the binaries formed during the computations are studied. The numerical results are discussed from the observational point of view.


2013 ◽  
Vol 9 (S302) ◽  
pp. 398-399
Author(s):  
L. Sabin ◽  
Q. Zhang ◽  
A. A. Zijlstra ◽  
N. A. Patel ◽  
R. Vázquez ◽  
...  

AbstractThe role of magnetic field in late type stars such as proto-planetary and planetary nebulae (PPNe/PNe), is poorly known from an observational point of view. We present submillimetric observations realized with the Submillimeter Array (SMA) which unveil the dust continuum polarization in the envelopes of two well known PPNe: CRL 618 and OH 231.8+4.2. Assuming the current grain alignment theory, we were then able to trace the geometry of the magnetic field.


2005 ◽  
Vol 38 (2) ◽  
pp. 157-160 ◽  
Author(s):  
ZEN KOMIYA ◽  
KIYOSHI KAWABATA ◽  
KOICHI HIRANO ◽  
HIROSHI BUNYA ◽  
NAOTAKA YAMAMOTO

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