@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},
 identifiers = {[object Object]},
 keywords = {Galaxies: evolution,Galaxies: fundamental parameters,Galaxies: general,Galaxies: peculiar,Galaxies: structure},
 pages = {340-356},
 volume = {394},
 websites = {http://mnras.oxfordjournals.org/cgi/doi/10.1111/j.1365-2966.2008.14292.x},
 month = {3},
 day = {21},
 id = {384f84c4-83e2-35f2-98bd-896d9349bb94},
 created = {2017-03-14T03:15:34.000Z},
 accessed = {2016-12-21},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-03-21T09:10:56.250Z},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {false},
 citation_key = {Garcia-Appadoo2009},
 notes = {NULL},
 private_publication = {false},
 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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