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Potential, velocity, and density fields from redshift-distance samples: Application - Cosmography within 6000 kilometers per secondA potential flow reconstruction algorithm has been applied to the real universe to reconstruct the three-dimensional potential, velocity, and mass density fields smoothed on large scales. The results are shown as maps of these fields, revealing the three-dimensional structure within 6000 km/s distance from the Local Group. The dominant structure is an extended deep potential well in the Hydra-Centaurus region, stretching across the Galactic plane toward Pavo, broadly confirming the Great Attractor (GA) model of Lynden-Bell et al. (1988). The Local Supercluster appears to be an extended ridge on the near flank of the GA, proceeding through the Virgo Southern Extension to the Virgo and Ursa Major clusters. The Virgo cluster and the Local Group are both falling toward the bottom of the GA potential well with peculiar velocities of 658 + or - 121 km/s and 565 + or - 125 km/s, respectively.
Document ID
19910031880
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Bertschinger, Edmund
(MIT Cambridge, MA, United States)
Dekel, Avishai
(Jerusalem, Hebrew University Israel)
Faber, Sandra M.
(Lick Observatory; California, University Santa Cruz, United States)
Dressler, Alan
(Carnegie Institution of Washington, Observatories, Pasadena CA, United States)
Burstein, David
(Arizona State University Tempe, United States)
Date Acquired
August 15, 2013
Publication Date
December 1, 1990
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 364
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A16503
Funding Number(s)
CONTRACT_GRANT: NSF AST-90-01762
CONTRACT_GRANT: NSF AST-87-02899
CONTRACT_GRANT: NSF PHY-82-17853
CONTRACT_GRANT: NSF PHY-88-00801
CONTRACT_GRANT: NAGW-1320
Distribution Limits
Public
Copyright
Other

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