@article{
 title = {A relation between the dark mass of elliptical galaxies and their shape},
 type = {article},
 year = {2014},
 identifiers = {[object Object]},
 keywords = {Dark matter,Galaxies:elliptical and lenticular:cD},
 pages = {1535-1551},
 volume = {438},
 websites = {https://arxiv.org/ftp/arxiv/papers/1304/1304.6932.pdf},
 id = {a540546f-e073-301f-a42e-b7890ed16199},
 created = {2017-09-20T00:48:38.411Z},
 accessed = {2017-09-19},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-09-20T00:54:46.494Z},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {false},
 citation_key = {Deur2014a},
 folder_uuids = {6f0ef382-5ddc-4c92-a313-25d73428afe8},
 private_publication = {false},
 abstract = {It has been reported that there appears to be little non-baryonic dark matter in some elliptical galaxies. We have studied a large number of elliptical galaxies and found a clear, previously unknown, correlation between their dark matter content and the ellipticity of their visible shape. At equal luminosities, flattened medium-size elliptical galaxies have on the average five times larger total mass than round ones. Such a correlation provides a new testing ground for models of dark matter and galaxy formation.},
 bibtype = {article},
 author = {Deur, A},
 journal = {Monthly Notices of the Royal Astronomical Society},
 number = {2}
}

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