@misc{
 title = {Properties of Elliptical Galaxies},
 type = {misc},
 websites = {http://www2.astro.psu.edu/users/rbc/a504/ellipticals.pdf,https://www.ifa.hawaii.edu/~barnes/ast626_05/peg.pdf},
 id = {af7ab5d6-81b9-3a5d-b38d-9f1ba022243d},
 created = {2017-08-30T00:50:32.167Z},
 accessed = {2017-06-08},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-08-30T00:59:14.873Z},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {true},
 citation_key = {Ciardullo},
 private_publication = {false},
 abstract = {In the last 20 years our notions about elliptical galaxies have changed radically; these galaxies are much more complex than they seemed at first. 3.1 Folklore & Mythology Traditionally, elliptical galaxies were seen as simple monolithic systems. Their overall luminosity profiles appeared to follow de Vaucouleurs' (1948) law, while their central regions fit the constant-density cores of King (1966) models. Elliptical galaxies were assumed to be oblate spheroids, flattened by rotation. The stars within them were thought to comprise a single, ancient population like the bulge and halo populations of our galaxy; gas and dust were thought to be absent. Finally, elliptical galaxies were considered to be relaxed and dynamically quiescent. At one level or another, all of the above are incorrect.},
 bibtype = {misc},
 author = {Barnes, Joshua E. and Ciardullo, Robin}
}

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