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Rotation curve

A final result of interest is the integral of the area under the transformed stiffness versus angle of rotation curve from <)) = 0 to <)) = 2k, that is, one complete revolution of the laminate ... [Pg.445]

It was noticed that the longer C-H distances are of little importance in the curve for the free-rotation model the curve calculated by ignoring all C-H terms except those for the bond distance and the next larger distance (which is unchanged by rotation) is qualitatively indistinguishable from the free-rotation curve, and the s values for the peaks of the two curves differ on the average by only 0.02. In our treatment of propane and isobutane we have made use of this simplification. [Pg.647]

Figure 1.8 Diastereoisomeric effects predicted to arise for coronene adsorption on Cu l 1 1 from a combination of molecular rotation (curved arrows) within the 2D adsorbate lattice to allow C—H bond interdigitation and the ( 19 X 19)R 23.4° lattice. The black arrows indicate a high symmetry within the molecule bisecting C—H bonds. Figure 1.8 Diastereoisomeric effects predicted to arise for coronene adsorption on Cu l 1 1 from a combination of molecular rotation (curved arrows) within the 2D adsorbate lattice to allow C—H bond interdigitation and the ( 19 X 19)R 23.4° lattice. The black arrows indicate a high symmetry within the molecule bisecting C—H bonds.
We present chemical evolution models for NGC 6822 computed with five fixed parameters, all constrained by observations, and only a free parameter, related with galactic winds. The fixed parameters are i) the infall history that has produced NGC 6822 is derived from its rotation curve and a cosmological model ii) the star formation history of the whole galaxy based on star formation histories for 8 zones inferred from H-R diagrams iii) the IMF, the stellar yields, and the percentage of Type la SNe progenitors are the same than those that reproduce the chemical history of the Solar Vicinity and the Galactic disk. [Pg.360]

The existence of dark matter (either baryonic or non-baryonic) is inferred from its gravitational effects on galactic rotation curves, the velocity dispersions and hydrostatic equilibrium of hot (X-ray) gas in clusters and groups of galaxies, gravitational lensing and departures from the smooth Hubble flow described by Eq. (4.1). This dark matter resides at least partly in the halos of galaxies such as our... [Pg.148]

Fig. 8.14. Surface densities of atomic and molecular hydrogen in the Galaxy as a function of Galactocentric distance the Sun is at 8.5 kpc. Beyond that distance, the deduced surface density depends on the assumed law of Galactic rotation KBH refers to Kulkarni, Blitz and Heiles (1982). Assuming their rotation curve, the total gas surface density falls by about a factor of 2 between 4.5 and 13 kpc, corresponding to an exponential fall-off with a scale length a l of about 12 kpc. After Dame (1993). Courtesy T.M. Dame. Fig. 8.14. Surface densities of atomic and molecular hydrogen in the Galaxy as a function of Galactocentric distance the Sun is at 8.5 kpc. Beyond that distance, the deduced surface density depends on the assumed law of Galactic rotation KBH refers to Kulkarni, Blitz and Heiles (1982). Assuming their rotation curve, the total gas surface density falls by about a factor of 2 between 4.5 and 13 kpc, corresponding to an exponential fall-off with a scale length a l of about 12 kpc. After Dame (1993). Courtesy T.M. Dame.
Selection of the material model is another important factor to be considered. Some programs allow the user to specify plastic moment-rotation curves for beam elements. However, the more rigorous and most widely available method of defining nonlinear material properties is to specify the stress versus strain data, Plastic behavior is approximated at the section level in the former method whereas, the latter method tracks plastic behavior at the individual integration points (fibers) through the thickness of the member. Each method has its advantages and disadvantages. [Pg.183]

The total mass of the Galaxy is about 10 Mq. Of this 10(X) billion solar masses, only about one-tenth is actually visible. This is what is implied by the Galaxy s rotation curve, i.e. the graph of its rotation speed at different distances from the centre. All other matter is therefore classed as dark matter. The mass of stars is thus about 100 billion solar masses, and the mass of interstellar material a few billion more. [Pg.110]

Note that the baryonic density of 2% to 5% is of the same order of magnitude as the galactic density indicated by rotation curves (viz. 5%). It is thus perfectly reasonable to suggest that a large part of galactic matter is located in compact massive objects (CMOs) assumed to swarm around the bright galactic disk. Will these compact massive objects remain forever hidden ... [Pg.201]

Figures 6 and 7 illustrate calculations which include the putative fast component. With kj/ks = 2 and appropriate rate constants for the formation (ks) and reversion to X (k7) of the fast component, this component would increase to nearly its equilibrium level in 3 minutes, overshoot, then slowly decline to equilibrium. The optical rotation curve computed on this basis (Figure 7) follows the experimental one very closely for the first 20 minutes. Figures 6 and 7 illustrate calculations which include the putative fast component. With kj/ks = 2 and appropriate rate constants for the formation (ks) and reversion to X (k7) of the fast component, this component would increase to nearly its equilibrium level in 3 minutes, overshoot, then slowly decline to equilibrium. The optical rotation curve computed on this basis (Figure 7) follows the experimental one very closely for the first 20 minutes.
For arabinose the half-times for all components are essentially the same. As long as this constraint is obeyed, the calculated optical rotation curves would be expected to show no rapid initial drop, and this is what was found. Therefore, we must postulate a fifth, as yet undetected, fast component in mutarotating arabinose solutions. Here the only reasonable... [Pg.38]

Fig. 18. Heat capacity of a cooperative system as a function of the excess energy on aggregation. The critical temperature of a First order transition is reached with the last curve (parameter = 454). The parameter 0 corresponds to an isolated hindered rotator. Curves after data of Ref.ll0b)... Fig. 18. Heat capacity of a cooperative system as a function of the excess energy on aggregation. The critical temperature of a First order transition is reached with the last curve (parameter = 454). The parameter 0 corresponds to an isolated hindered rotator. Curves after data of Ref.ll0b)...
The second is using the Tully-Fisher relationship, which provides a direct relationship between the absolute luminosity of a spiral galaxy and its maximum rotation speed. Since the maximum rotation speed can be directly estimated by observation, one can estimate the absolute luminosity since we measure directly the apparent luminosity, the inverse-square law allows us to estimate the distance to the object concerned. For the present discussion, it is important to understand that, at optical wavelengths, estimates of maximum rotation speeds are generally extrapolations from rotation curve measurements. [Pg.300]

The rotation curve is calculated in two steps (1) by subtracting the global redshift component (i.e., cosmological redshift + Doppler effect arising from peculiar motion) from the Doppler profile measured directly across the galaxy s disk and (2) by determining the actual dynamical centre of the galaxy. [Pg.300]

The process of estimating the global redshift component and estimating the dynamical center is termed the process of folding the rotation curve. Because of the very noisy nature of the data, this process is very far from trivial, especially if one is interested in accurate dynamical studies of spiral galaxies. [Pg.300]

While this subjective approach was perfectly justifiable for a small experimental analysis, it could play no part in the large analysis contemplated for which all decisions had to be made in an automatic blackbox fashion. We dealt with this problem by writing a piece of software that automatically cut out the innermost parts of rotation curves that were judged, according to objectively defined statistical criteria, to be unusually affected by the presence of the bulge. The effectiveness of this process was tested by means completely independent of the present considerations. [Pg.305]

The primary task was to test the power law hypothesis, and to this end I had obtained a sample of 900 optical rotation curves, originally measured by Mathewson et al. [9], and folded (see Section II.D) by Persic and Salucci [10], two Italian astronomers. [Pg.305]

With this information, the results of the primary analysis of the 900 rotation curves made it possible to recalibrate the Table I to give specific predictions for the existence of preferred In A values in the folded MFB sample, and these predictions are given in Table II. [Pg.305]

Table II represents a set of specific predictions about the In A distribution for the 900 folded MFB rotation curves, and it is these that were to be tested against the MFB sample. Table II represents a set of specific predictions about the In A distribution for the 900 folded MFB rotation curves, and it is these that were to be tested against the MFB sample.
The folding of each rotation curve (see Section II.D). This data reduction process is nontrivial, and different people have their own favored methods. [Pg.306]

These rotation curves were folded by the Italian astronomers Persic and Salucci [10] using a case-by-case eyeball technique. The short vertical bars give the positions of the predicted peak centers given in Table II, and it is... [Pg.306]

For completeness, we show, in Fig. 3, the In A frequency diagram for the rotation curves of the MFB sample (originally folded by Persic and Salucci [10]) folded by this automatic method the vertical dotted lines indicate the peak centers of the Persic-Salucci solution. The clarity with which the peaks in this latter solution are reproduced in Fig. 3 indicates (1) that the peaks of Fig. 2 are not an artifact of the Persic-Salucci method and (2) that the automatic algorithm works. [Pg.307]

The next sample of 1200+ rotation curves was observed by the Australians, Mathewson and Ford (MF) [13] (Buchhorn had discovered that astronomy pays... [Pg.307]


See other pages where Rotation curve is mentioned: [Pg.259]    [Pg.263]    [Pg.323]    [Pg.63]    [Pg.197]    [Pg.225]    [Pg.32]    [Pg.37]    [Pg.297]    [Pg.299]    [Pg.300]    [Pg.303]    [Pg.304]    [Pg.304]    [Pg.305]    [Pg.306]    [Pg.306]   
See also in sourсe #XX -- [ Pg.110 , Pg.197 ]




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