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Branching radial

Recent intense research efforts have focused on the synthesis of multi-branched polymers (i.e., cascade molecules) that can be characterized by their uniform branching, radial symmetry, dense packing, entanglement-free globular shapes, and large number of chain ends at their peripheries. [Pg.101]

TroUsas, M., Hawker, C.J., Remenar, J.F. et al. (1998b) Highly branched radial block copolymers via dendritic initiation of aUphatic polyesters. Journal of Polymer Science Part A-Polymer Chemistry, 36,2793-2798. [Pg.166]

Fig. 5.1. The three domains of life in a radial time sequence based on genetic (RNA) analysis. The distinction between anaerobes and aerobes is not made here and the branching to eukaryotes is left unclear. All the domains advanced with time but in very different ways (see Woese, C. (1998) in Further Reading, and Sogin, M. (1993), Science, 260, 340). Note the general gene transfer in prokaryotes and to eukaryotes (see Chapter 7). Fig. 5.1. The three domains of life in a radial time sequence based on genetic (RNA) analysis. The distinction between anaerobes and aerobes is not made here and the branching to eukaryotes is left unclear. All the domains advanced with time but in very different ways (see Woese, C. (1998) in Further Reading, and Sogin, M. (1993), Science, 260, 340). Note the general gene transfer in prokaryotes and to eukaryotes (see Chapter 7).
The DART large programme at ESO made v ei and [Fe/H] measurements from FLAMES spectroscopy of 401 red giant branch (RGB) stars in the Sculptor (Scl) dSph [6]. The relatively high signal/noise, S/N ( 10-20 per pixel) resulted in both accurate metallicities ( 0.1 dex from internal errors) and radial velocities ( 2 km/s). This is the first time that a large sample of accurate velocities and metallicities have been measured in a dwarf galaxy. [Pg.214]

Abstract. We present the results of a spectroscopic analysis of bright stars in the Carina dSph galaxy. We collected low-resolution FORS2 VLT spectra of ss 200 stars. Our spectroscopic targets have been selected among the evolved Carina stars, in particular we selected low-mass, old Red Giant, Asymptotic, and Horizontal Branch stars, as well as intermediate-age stars of the Red Clump. We present preliminary estimates concerning the radial velocities of old and intermediate-age populations. [Pg.272]

They therefore finally appear as polyhedra. Because of their radial growth the fibrillar or lamellar crystals have only little space-filling ability as they move away from the central nucleus. Typically for spherulitic structures, an irregular noncrystallo-graphic branching usually at small angles can be observed. [Pg.296]

Classically the liver has been divided into hexagonal lobules centred around the terminal hepatic venules. Blood enters the liver through the portal tracts that are situated at the corners of the hexagon. The portal tracts are triads of a portal vein, an hepatic artery, and a common hepatic bile duct. The vast expanse of hepatic tissue, mostly consisting of parenchymal cells (PC) or hepatocytes, is serviced via terminal branches of the portal vein and hepatic artery, which enters the tissue at intervals. The hepatocytes are organized into cords of cells radially disposed about the central hepatic venule. Between these cords are vascular sinusoids that transport the blood to the central hepatic venules. The blood is collected through the hepatic venules into the hepatic vein which exits the liver into the inferior vena cava (Figure 4.1). [Pg.90]

Sade LE, Kanzaki H, Severyn D, Dohi K, Gorcsan J, III. Quantification of radial mechanical dyssynchrony in patients with left bundle branch block and idiopathic dilated cardiomyopathy without conduction delay by tissue displacement imaging. Am. J. Cardiol. 2004 94 514-8. [Pg.65]

Fig. 9. Drawing of a 2D projection of a spherulite formed from radially grown lamellae with a small degree of branching... Fig. 9. Drawing of a 2D projection of a spherulite formed from radially grown lamellae with a small degree of branching...

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See also in sourсe #XX -- [ Pg.203 , Pg.297 ]




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