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Mapping the Local Structure

Published online by Cambridge University Press:  23 September 2016

R. Brent Tully
R. Brent Tully*
Affiliation:
University of Hawaii, 2680 Woodlawn Dr., Honolulu HI 96822, USA

Abstract

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A database of 30,000 galaxies within a cube ±8,000 km s--1 centered at our position is used to illustrate the properties of the nearby structure in the distribution of galaxies. The data cube can be manipulated in ways that enhance the visualization of the structure with special software. The dominant regions of high density are the Great Attractor, the Great Wall, and the Perseus-Pisces complexes. There are many voids.

Information

Type
Session III: Local Structure
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005, pp. 190 - 195
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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