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Galaxy Surface Brightness and Clustering: A Test for Biased Galaxy Formation Scenarios?

Djorgovski, S. and Davis, Marc (1986) Galaxy Surface Brightness and Clustering: A Test for Biased Galaxy Formation Scenarios? In: Galaxy Distances and Deviations from Universal Expansion. NATO ASI Series. No.180. Springer , Dordrecht, pp. 291-294. ISBN 978-94-010-8591-5. https://resolver.caltech.edu/CaltechAUTHORS:20190730-135459615

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Abstract

Davis & Djorgovski (1985) described a correlation, between the clustering properties and characteristic surface brightness of UGC galaxies. The existence of such an effect is of considerable importance for theories of galaxy formation. In this contribution., we are trying to clarify some questions and problems about this intriguing phenomenon.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-009-4702-3_49DOIArticle
ORCID:
AuthorORCID
Djorgovski, S.0000-0002-0603-3087
Additional Information:© 1986 D. Reidel Publishing Company. We acknowledge stimulating discussions with G. Bothun and M. Geller. This work was supported in part by the NSF grant AST-8419910.
Funders:
Funding AgencyGrant Number
NSFAST-8419910
Subject Keywords:Surface Brightness; Galaxy Formation; Redshift Distribution; Redshift Survey; Local Supercluster
Series Name:NATO ASI Series
Issue or Number:180
DOI:10.1007/978-94-009-4702-3_49
Record Number:CaltechAUTHORS:20190730-135459615
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190730-135459615
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97526
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:01 Aug 2019 20:22
Last Modified:16 Nov 2021 17:32

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