Published March 15, 1987
| Published
Journal Article
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Interpretation of large-scale deviations from the Hubble flow
Abstract
The theoretical expectation for large-scale streaming velocities relative to the Hubble flow is expressed in terms of statistical correlation functions. Only for objects that trace the mass would these velocities have a simple cosmological interpretation. If some biasing effects the objects' formation, then nonlinear gravitational evolution is essential to predicting the expected large-scale velocities, which also depend on the nature of the biasing.
Additional Information
© 1987 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1986 June 20; accepted 1986 September 9. Work supported in part by the US Department of Energy under contract DEAC03-81-ER40050. Supported in part by US Department of Energy Outstanding Junior Investigator Program under contract DE-FG03-84-ER40172.Attached Files
Published - 1987ApJ___314__431G.pdf
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Additional details
- Eprint ID
- 70895
- Resolver ID
- CaltechAUTHORS:20161005-153314099
- DE-FG03-84-ER40172
- Department of Energy (DOE)
- DE-AC03-81-ER40050
- Department of Energy (DOE)
- Created
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2016-10-05Created from EPrint's datestamp field
- Updated
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2021-11-11Created from EPrint's last_modified field