@article{
 title = {Distribution and motions of atomic hydrogen in lenticular galaxies. XI - A summary of H I observations and evolutionary scenarios},
 type = {article},
 year = {1991},
 identifiers = {[object Object]},
 keywords = {Barred Galaxies,Gas Dynamics,H I Regions,Hydrogen Atoms,Interstellar Gas,Lenticular Bodies,Mass To Light Ratios,Spiral Galaxies,Star Formation Rate},
 pages = {71-92},
 volume = {243},
 id = {f51f6456-fa11-3412-98eb-f77b2a03ce38},
 created = {2017-02-11T07:57:39.000Z},
 accessed = {2017-02-10},
 file_attached = {true},
 profile_id = {d9ca9665-cda3-3617-b3e8-ecfc7a8d9739},
 group_id = {5a95a0b6-1946-397c-b16a-114c6fdf3127},
 last_modified = {2017-07-29T20:40:44.130Z},
 tags = {IEG-HI-paper2},
 read = {false},
 starred = {false},
 authored = {false},
 confirmed = {true},
 hidden = {false},
 citation_key = {VanDriel1991},
 notes = {NULL},
 folder_uuids = {775a297d-19cf-4810-acfc-68632a86c3b1},
 private_publication = {false},
 abstract = {It is considered that the H I velocity fields in most early-type galaxies can be described by circular rotation, sometimes in a considerably warped H I distribution. The derived rotation curves are essentially flat, sometimes out to 10 optical disk scale lengths, denoting the presence of massive dark halos, which is substantiated by detailed disk/bulge/halo mass model fits to the surface photometry and rotation curves of 3 galaxies. The most probable origins of the H I gas in SO galaxies seem to be either accretion from another galaxy, though not in the recent past, or a burnt-out disk scenario, for the lenticulars with an outer H I ring, where the denser inner H I disk has been consumed in star formation.},
 bibtype = {article},
 author = {van Driel, W. and van Woerden, H.},
 journal = {Astronomy & Astrophysics}
}

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