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oai:www.ideals.illinois.edu:2142/85191 2023-07-11 col_2142_5131 col_2142_14807 com_2142_5130 com_2142_14806 com_2142_8903

Lo, K.Y. Young, Lisa Marie 2015-09-25T22:35:40Z 2015-09-25T22:35:40Z 10000-01-01 1997 1997 The distribution and kinematics of HI in the dwarf ellipticals NGC 185 and NGC 205 are significantly different from those in giant ellipticals, so that an internal origin for the gas in the dwarf ellipticals should be considered. Finally, the presence of gas in LGS 3 conflicts with evolutionary models which predict that a burst of star formation activity should have removed all the gas from that galaxy. Made available in DSpace on 2015-09-25T22:35:40Z (GMT). No. of bitstreams: 2 license.txt: 4848 bytes, checksum: 96035ab3f5e1c23cc7138a224ce498bd (MD5) 9737299.pdf: 8892389 bytes, checksum: d45a136aa7c585db5ef45da75d77bc53 (MD5) Previous issue date: 1997 Embargo set by: Seth Robbins for item 86472 Lift date: Forever Reason: Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs U of I Only 167 p. Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1997. http://hdl.handle.net/2142/85191 (MiAaPQ)AAI9737299 eng Physics, Astronomy and Astrophysics Properties and Kinematics of the Interstellar Medium in a Small Sample of Nearby Dwarf Galaxies text Astronomy Astronomy University of Illinois at Urbana-Champaign Dissertation Ph.D.