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Central surface brightness

Scl is a close companion of the Milky Way, at a distance of 72 5 kpc [7], with a low total (dynamical) mass, (1.4 0.6) x 107Mq [8], and modest luminosity, My = —10.7 0.5, and central surface brightness, Soy = 23.5 0.5 mag/arcsec2 [9] with no HI gas [10]. CMD analysis, including the oldest Main Sequence turnoffs, has determined that this galaxy is predominantly old and that the entire star formation history can have lasted only a few Gyr [11]. [Pg.214]

The radial profiles were fit by a simultaneous minimization with respect to the four parameters the exponential disk scale length and central surface brightness, Vd and fid, and the bulge effective radius and surface brightness, and fig. Before fitting, each of the two components was convolved with a gaussian PSF, the parameters of which were determined from stars in the source frame or from standard star observations. [Pg.130]

Parameters of dynamically hot galaxies , i.e. various classes of ellipticals and the bulges of spirals, generally lie close to a Fundamental Plane in the 3-dimensional space of central velocity dispersion, effective surface brightness and effective radius or equivalent parameter combinations (Fig. 11.10). This is explained by a combination of three factors the Virial Theorem, some approximation to... [Pg.356]

For a subsample of 16 galaxies for which the surface brightness profiles cotdd be fitted well by an exponential, we have determined the B-E color in the center, at te,Ki and at 3 as, and looked at the inclination dq>endence of these colors. The data seem to indicate that the central area, including the region around re, is optically thick in B. At 3 as (arotmd D2s,b) the obscuration apparently is much less. [Pg.150]

Throughout the final phases, the solar wind will sweep across the Earth, tearing up the surface. The atoms of our dead will be driven from below and returned to the Sun. The Earth will surrender her dead. Finally, lit up by the bright white glare of the central star, the ejected matter will blossom into a beautiful planetary nebula rather like the one that so delightfully ornaments the constellation of the Lyre. The atoms of all human beings will shine in the sky, mixed with those of the animals and the stones. [Pg.133]

Fig. 16. Electrochemical impedance and fluorescence data for DNA modified Si(lll) upon hybridization and de-hybridization. The real (a) and imaginary (b) parts of the impedance (sample biased into depletion) are shown as a function of frequency. The various curves show the response of the initial surface modified with single stranded DNA (16-mer), after exposure to the complementary sequence S2 and de-hybridization. Exposure to a non-complementary sequence S3, did not significantly change the impedance. A plot of the real versus imaginary parts of the admittance is shown in (c), more clearly showing the hybridization induced changes. The fluorescence image shown in (d) confirms hybridization and de-hybridization, the central bright region corresponds to the area of the sample exposed to the DNA solution in the electrochemical cell. Reprinted from [93]. Fig. 16. Electrochemical impedance and fluorescence data for DNA modified Si(lll) upon hybridization and de-hybridization. The real (a) and imaginary (b) parts of the impedance (sample biased into depletion) are shown as a function of frequency. The various curves show the response of the initial surface modified with single stranded DNA (16-mer), after exposure to the complementary sequence S2 and de-hybridization. Exposure to a non-complementary sequence S3, did not significantly change the impedance. A plot of the real versus imaginary parts of the admittance is shown in (c), more clearly showing the hybridization induced changes. The fluorescence image shown in (d) confirms hybridization and de-hybridization, the central bright region corresponds to the area of the sample exposed to the DNA solution in the electrochemical cell. Reprinted from [93].
The coordination of DABCO to a central zinc ion was directly observed for a zinc porphyrin derivative (ZnTBPP)-adsorbed onto an Ag(100) surface in UHV [145], The central dark part of each ZnTBPP was capped by the coordination of a DABCO molecule, resulting in a bright spot in the center. [Pg.158]

Fig. 6. Low energy electron diffraction patterns at normal incidence from clean tungsten surfaces, (a) Ball model of W(llO) face. Some of the net lines (hk) are indexed in terms of a centered rectangular unit mesh (outlined), (b) Clean W(llO), 75 V. Diffuse brightness and central bright spot are caused by light from electron gun filament, (c) Clean W(llO), 300 V. (d) Ball model of (112) surface, the third densest of the boo lattice, (e) Clean W(112) at 90 V. Note the asymmetric intensities of the A/c and hA beams. The unit mesh contains only a single mirror plane perpendicular to surface. There is a strong scattering contribution from the exposed second layer which is asymmetrically positioned. Fig. 6. Low energy electron diffraction patterns at normal incidence from clean tungsten surfaces, (a) Ball model of W(llO) face. Some of the net lines (hk) are indexed in terms of a centered rectangular unit mesh (outlined), (b) Clean W(llO), 75 V. Diffuse brightness and central bright spot are caused by light from electron gun filament, (c) Clean W(llO), 300 V. (d) Ball model of (112) surface, the third densest of the boo lattice, (e) Clean W(112) at 90 V. Note the asymmetric intensities of the A/c and hA beams. The unit mesh contains only a single mirror plane perpendicular to surface. There is a strong scattering contribution from the exposed second layer which is asymmetrically positioned.
A spectacular example of a ridge and valley textile structure, 320 m in length, covers the central concourse of Denver Airport Terminal (1994) and is intended to mirror the snow-capped Rocky Mountains in the distance (Brown, 1994). This is a double-layer membrane used to improve the thermal and acoustic performance of the space (Berger, 2000, pp. 220-221). It is particularly employed to reduce the impact of aircraft engine noise on the interior. As Fig. 7.12 shows, here the distinct contrast between the bright membrane (bright, even though it is double-layer) and the duller surfaces at concourse level can clearly be seen, as discussed previously in Section 7.6.2. [Pg.245]


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