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Quantitative Study of Galaxy Morphology

Džanović, Dajana and Sharples, R. M. and Benson, A. J. and Frenk, C. S. (2003) Quantitative Study of Galaxy Morphology. Astrophysics and Space Science, 285 (1). pp. 73-77. ISSN 0004-640X. https://resolver.caltech.edu/CaltechAUTHORS:20191127-110317134

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Abstract

We use an automatic algorithm to fit two-dimensional bulge and disk surface brightness profiles to a sample of 200 Sloan Digital Sky Survey Early Data Release (SDSS EDR) galaxies of known redshift and brighter than r = 16. The bulge-to-disk (B/D) luminosity ratios can be combined with an estimate of the galaxy's local environment to address a number of key issues that are central to our understanding of galaxy formation: – How do B/D ratios depend upon galaxy luminosity? – What are the disk and spheroid luminosity functions for field galaxies? – How does the total luminosity in bulges and disks depend on environment?


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1023/a:1024601524412DOIArticle
https://rdcu.be/bXLAuPublisherFree ReadCube access
ORCID:
AuthorORCID
Benson, A. J.0000-0001-5501-6008
Additional Information:© 2003 Kluwer Academic Publishers. We would like to use this opportunity to thank JENAM 2002 GE Workshop organisers for their endless patience prior to submitting this work. It truly has been a great pleasure to take part in the Workshop and extremely exciting to visit the city of Porto – muito obrigada!
Subject Keywords:galaxies; galaxy morphologies; galaxy evolution
Issue or Number:1
Record Number:CaltechAUTHORS:20191127-110317134
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191127-110317134
Official Citation:Džanović, D., Sharples, R., Benson, A. et al. Astrophysics and Space Science (2003) 285: 73. https://doi.org/10.1023/A:1024601524412
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100101
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:27 Nov 2019 19:24
Last Modified:27 Nov 2019 19:24

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