986 resultados para Durand, A. B. (Asher Brown), 1796-1886.
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In hebr. Schr.
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von Joseph Klar
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In hebr. Schr.
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"Printed for the Committee."
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Microfilm.
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Mode of access: Internet.
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Mode of access: Internet.
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Mode of access: Internet.
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"The Anatomy of Man's Body" on page [3] is the only illustration.
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Introducción Desde la publicación, en 1866, de un artículo escrito por Dudley Baxter, titulado la expansión de los ferrocarriles y sus resultados, el problema del impacto que innovaba de los ferrocarriles e las economías centrales (particularmente Gran Bretaa y Estados Unidos), ha pasado a un primer plano. Posteriormente, y dentro del esquema teórico- metodológico elaborado por el New Economic History, en Estados Unidos, la edición de un difícil libro preparado por RW. Fogel imprimió a la cuestión su verdadero significado.
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The vocalizations of Hypsiboas ericae (Caramaschi & Cruz, 2000) are described and new information on the external morphology and osteology of the species are presented. H. ericae presents a bony spine in the prepolex and the individuals can present green or brown dorsal color, as other species of the Hypsiboas pulchellus (Duméril & Bibron, 1841) species group. The vocalizations of H. ericae are similar to the vocalizations of Hypsiboas bischoffi (Boulenger, 1887), Hypsiboas guentheri (Boulenger, 1886), and other species in the H. polytaenius (Cope, 1870 "1869") clade of the H. pulchellus species group, but some osteological aspects are different to those found in the majority of the species of this group.
SSSPM J1102-3431 brown dwarf characterization from accurate proper motion and trigonometric parallax
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Context. In 2005, Scholz and collaborators discovered, in a proper motion survey, a young brown dwarf SSSPM J1102-3431 (SSSPM J1102) of spectral type M8.5, probable member of the TW Hydrae Association and possible companion of the T Tauri star TWHya. The physical characterization of SSSPM J1102 was based on the hypothesis that it forms a binary system with TWHya. The recent discovery of a probable giant planet with a very short-period inside the TW Hya protoplanetary disk, as well as a disk around SSSPM J1102, make it especially interesting and important to measure well the physical parameters of SSSPM J1102. Aims. Trigonometric parallax and proper motion measurements of SSSPM J1102 are necessary to test for TWA membership and, thus, to determine the mass and age of this young brown dwarf and the possibility that it forms a wide binary system with TW Hya. Methods. Two years of regular observations at the ESO NTT/SUSI2 telescope have enabled us to determine the trigonometric parallax and proper motion of SSSPM J1102. Results. With our accurate distance determination of 55.2(-1.4)(+1.6) pc and proper motions of (-67.2, -14.0) +/- 0.6 mas/yr, we could confirm SSSPM J1102 as a very probable member of TWA. Assuming the TW Hydrae association age of 5-10 Myr, the evolutionary models compared to the photometry of this young brown dwarf indicate a mass of M = 25 +/- 5 M(Jup) and an effective temperature T(eff) = 2550 +/- 100 K. Conclusions. Our parallax and proper motion determination allow us to precisely describe the physical properties of this low mass object and to confirm its TWA membership. Our results indicate that SSSPMJ1102 may be a very wide separation companion of the star TW Hya.