Correlations among the properties of galaxies found in a blind H i survey, which also have SDSS optical data. Garcia-Appadoo, D., A., West, A., A., Dalcanton, J., J., Cortese, L., & Disney, M., J. Monthly Notices of the Royal Astronomical Society, 394(1):340-356, 3, 2009.
Paper
Website abstract bibtex We have used the Parkes Multibeam system and the Sloan Digital Sky Survey (SDSS) to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases against unevolved or low surface brightness objects. For each source 9 intrinsic properties are measured homogeneously, as well as inclination and an optical spectrum. The sample, which should be almost entirely free of either misidentification or confusion, includes a wide diversity of galaxies ranging from inchoate, low surface brightness dwarfs to giant spirals. Despite this diversity there are 5 clear correlations among their properties. They include a common dynamical mass-to-light ratio within their optical radii, a correlation between surface-brightness and Luminosity and a common HI surface-density. Such correlation should provide strong constrains on models of galaxy formation and evolution.
@article{
title = {Correlations among the properties of galaxies found in a blind H i survey, which also have SDSS optical data},
type = {article},
year = {2009},
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abstract = {We have used the Parkes Multibeam system and the Sloan Digital Sky Survey (SDSS) to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases against unevolved or low surface brightness objects. For each source 9 intrinsic properties are measured homogeneously, as well as inclination and an optical spectrum. The sample, which should be almost entirely free of either misidentification or confusion, includes a wide diversity of galaxies ranging from inchoate, low surface brightness dwarfs to giant spirals. Despite this diversity there are 5 clear correlations among their properties. They include a common dynamical mass-to-light ratio within their optical radii, a correlation between surface-brightness and Luminosity and a common HI surface-density. Such correlation should provide strong constrains on models of galaxy formation and evolution.},
bibtype = {article},
author = {Garcia-Appadoo, D. A. and West, A. A. and Dalcanton, J. J. and Cortese, L. and Disney, M. J.},
journal = {Monthly Notices of the Royal Astronomical Society},
number = {1}
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