dc.citation.endPage |
30 |
- |
dc.citation.number |
1 |
- |
dc.citation.startPage |
25 |
- |
dc.citation.title |
Publications of The Korean Astronomical Society |
- |
dc.citation.volume |
7 |
- |
dc.contributor.author |
Ryu, Dongsu |
- |
dc.date.accessioned |
2023-12-22T13:06:58Z |
- |
dc.date.available |
2023-12-22T13:06:58Z |
- |
dc.date.created |
2015-08-28 |
- |
dc.date.issued |
1992-12 |
- |
dc.description.abstract |
Recent redshift surveys suggest that most galaxies may be distributed on the surfaces of bubbles surrounding large voids. To investigate the quantitative consistency of this qualitative picture of large-scale structure, we study analytically the clustering properties of galaxies in a universe filled with spherical shells. In this paper, we report the results of the calculations for the spatial and angular two-point correlation functions of galaxies. With of galaxies in clusters and a power law distribution of shell sizes, , , the observed slope and amplitude of the spatial two-point correlation function can be reproduced. (It has been shown that the same model parameters reproduce the enhanced cluster two-point correlation function, ). The corresponding angular two-point correlation function is calculated using the relativistic form of Limber's equation and the Schecter-type luminosity function. The calculated w() agrees with the observed one quite well on small separations (). |
- |
dc.identifier.bibliographicCitation |
Publications of The Korean Astronomical Society, v.7, no.1, pp.25 - 30 |
- |
dc.identifier.issn |
1225-1534 |
- |
dc.identifier.uri |
https://scholarworks.unist.ac.kr/handle/201301/16392 |
- |
dc.identifier.url |
http://www.koreascience.or.kr/article/ArticleFullRecord.jsp?cn=CMHHCI_1992_v7n1_25&ordernum=10 |
- |
dc.language |
영어 |
- |
dc.publisher |
한국천문학회 |
- |
dc.title |
GALAXY CORRELATION IN A BUBBLY UNIVERSE |
- |
dc.type |
Article |
- |
dc.description.journalRegisteredClass |
other |
- |