Hostname: page-component-8448b6f56d-qsmjn Total loading time: 0 Render date: 2024-04-19T16:14:25.088Z Has data issue: false hasContentIssue false
  • English
  • Français

The Space Distribution of Local Radio and X-ray Galaxies

Published online by Cambridge University Press:  25 April 2016

P. A. Shaver
P. A. Shaver*
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-8046 Garching bei München, FRG
Get access Rights & Permissions [Opens in a new window]

Extended abstract

Local large scale structure is best studied using statistically complete samples which cover the entire sky, and for which full redshift information is available. The optical galaxy redshift surveys which have been made to date involve many thousands of objects but cover only limited parts of the sky, and so provide only a fragmented picture of local large scale structure. Complete samples of radio and X-ray galaxies are available, however, with large sky coverage. While the number of objects is small, they may still suffice to define the dominant local structures, particularly as they may preferentially sample the deeper gravitational potentials and so provide a more efficient tracer of dominant structure.

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 3 , 1990 , pp. 250 - 251
Copyright
Copyright © Astronomical Society of Australia 1990

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Lahav, O., Edge, A. C., Fabian, A. C. and Putney, A., 1989, preprint.Google Scholar
Large, M. I., Mills, B. Y., Little, A. G., Crawford, D. F. and Sutton, J. M., 1981, Mon. Not. R. Astron. Soc., 194, 693.Google Scholar
Piccinotti, G., Mushotzky, F. F., Boldt, E. A., Holt, S. S., Marshall, F. E., Serlemitsos, P. J. and Shafer, R. A., 1982, Astrophys. J., 253, 485.Google Scholar
Shaver, P. A. and Pierre, M., 1989, Astron. Astrophys., 220, 35.Google Scholar
Wall, J. V. and Peacock, J. A., 1985, Mon. Not. R. Astron. Soc., 216, 173.Google Scholar