The apparent and intrinsic shape of the APM galaxy clusters
- 21 August 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 316 (4), 779-785
- https://doi.org/10.1046/j.1365-8711.2000.03590.x
Abstract
No abstract availableKeywords
This publication has 27 references indexed in Scilit:
- Galaxy clusters: oblate or prolate?Monthly Notices of the Royal Astronomical Society, 2000
- 0 and substructure in galaxy clustersMonthly Notices of the Royal Astronomical Society, 1998
- The APM Galaxy Survey -- V. Catalogues of galaxy clustersMonthly Notices of the Royal Astronomical Society, 1997
- X-Ray Constraints on the Intrinsic Shapes and Baryon Fractions of Five Abell ClustersThe Astrophysical Journal, 1996
- The shapes of galaxy clustersMonthly Notices of the Royal Astronomical Society, 1995
- The reliability of X-ray constraints of intrinsic cluster shapesThe Astrophysical Journal, 1995
- A Morphology-Cosmology Connection for X-Ray ClustersThe Astrophysical Journal, 1993
- Gravitational clustering from scale-free initial conditionsMonthly Notices of the Royal Astronomical Society, 1988
- The formation of dark halos in a universe dominated by cold dark matterThe Astrophysical Journal, 1988
- The morphology of clusters of galaxiesMonthly Notices of the Royal Astronomical Society, 1980