894 resultados para Anglo-Saxons


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Founded by W. Hadfield and C. Dunlop and for many years edited by the latter.

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In 3 parts: the 1st an abridgment of Geoffrey of Monmouth's "Historia Britonum": the 2d, a history of the Anglo-Saxon and Norman kings to the death of Henry III; the 3d, a history of the reign of Edward I. The language is a specimen of the French of Yorkshire. cf. Introd.

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"Glossary of Anglo-Norman and Gascon words": p. [145]-197; "Glossary of Catalan words": p. [199]-238; "Glossary of Low-German words": p. [239]-262.

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Mode of access: Internet.

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Mode of access: Internet.

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Among friends.--The Anglo-American school of polite unlearning.--The hundred worst books.--The convention of books.--In praise of politicians.--My missionary life in Persia.--The colonel in the theological seminary.--The romance of ethics.--The merry devil of education.

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The road.--The sacred work.--Balance sheet of the soldier workman.--The children's jewel fund.--France, 1916-1917--an impression.--Englishman and Russian.--American and Briton.--Anglo-American drama and its future.--Speculations.--The land, 1917.--The land, 1918.--Grotesques.

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Includes section "Book reviews".

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Includes bibliographical references and index.

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"It is proposed by the Society, in continuing the work, to trace down the stream of British literature, in successive periods of time, to the close of the seventeenth century." Only these two volumes appeared, however.

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"The first, third, tenth and fifteenth chapters in the present volume have seen the light already in ʻthe Nineteenth century'; the ninth is re-arranged from ʻthe Anglo-Saxon review'; and the sixteenth reprinted from ʻthe Magazine of fine arts' ... Certain of the remarks in other portions of this book were first made in the ʻStandard'."--Note.

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"The first, third, tenth and fifteenth chapters in the present volume have seen the light already in 'the Nineteenth century'; the ninth is re-arranged from 'the Anglo-Saxon review'; and the sixteenth reprinted from 'the Magazine of fine arts' ... Certain of the remarks in other portions of this book were first made in the 'Standard.'"--Note.

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We present results from a pilot study of a new wide-field, multicolour (BVR) CCD imaging project, designed to examine galaxy evolution along large-scale filaments that connect clusters of galaxies at intermediate redshifts (0.07 < z < 0.20). Our pilot data set is based on 0.56 deg(2) of observations targeted on Abell 1079 and Abell 1084 using the Wide Field Imager on the Anglo-Australian Telescope. We describe our data reduction pipeline and show that our photometric error is 0.04 mag. By selecting galaxies that lie on the colour-magnitude relation of the two clusters we verify the existence of a low-density (similar to3-4 Mpc(-2)) filament population, conjoining them at a distance of > 3r(Abell) from either cluster. By applying a simple field correction, we characterize this filament population by examining their colour distribution on a (V-R)-(B-V) plane. We confirm the galaxian filament detection at a 7.5 sigma level using a cut at M-V = -18 and we discuss their broad properties.

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We present 547 optical redshifts obtained for galaxies in the region of the Horologium-Reticulum supercluster (HRS) using the 6 degrees field (6dF) multifiber spectrograph on the UK Schmidt Telescope at the Anglo-Australian Observatory. The HRS covers an area of more than 12 degrees x 12 degrees on the sky centered at approximately alpha = 03(h)19(m), delta = 50 degrees 02'. Our 6dF observations concentrate on the intercluster regions of the HRS, from which we describe four primary results. First, the HRS spans at least the redshift range from 17,000 to 22,500 km s(-1). Second, the overdensity of galaxies in the intercluster regions of the HRS in this redshift range is estimated to be 2.4, or delta rho/(rho) over bar similar to 1: 4. Third, we find a systematic trend of increasing redshift along a southeast-northwest spatial axis in the HRS, in that the mean redshift of HRS members increases by more than 1500 km s(-1) from southeast to northwest over a 12 degrees region. Fourth, the HRS is bimodal in redshift with a separation of similar to 2500 km s(-1) (35 Mpc) between the higher and lower redshift peaks. This fact is particularly evident if the above spatial-redshift trend is fitted and removed. In short, the HRS appears to consist of two components in redshift space, each one exhibiting a similar systematic spatial-redshift trend along a southeast-northwest axis. Lastly, we compare these results from the HRS with the Shapley supercluster and find similar properties and large-scale features.