@misc{
 title = {Chapter 6: Spiral Galaxies},
 type = {misc},
 websites = {http://www.usm.lmu.de/~jmohr/Essentials2012/06_spirals.pdf},
 id = {9f2c98dc-81f9-35a7-a8ee-a9fc02c12093},
 created = {2017-03-14T04:20:57.000Z},
 accessed = {2017-01-30},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-06-20T22:27:45.409Z},
 tags = {globular cluster distribution},
 read = {true},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {true},
 citation_key = {Mohr},
 notes = {A good summary at a intro graduate level of galaxy properties. Gave special attention to the brief discussion on globular clusters on slide #7 which provided a globular cluster number density profile relation (as a function of radius), which could be used later in comparing globular cluster distributions of IEGs using HST data.},
 folder_uuids = {5cebd862-8031-4107-83be-d95baa57e832},
 private_publication = {false},
 bibtype = {misc},
 author = {Mohr, Joseph}
}

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