Computer Science
Scientific paper
Feb 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002noao.prop..246w&link_type=abstract
NOAO Proposal ID #2002A-0246
Computer Science
Scientific paper
Dwarf galaxies are central to theories of galaxy formation, contributing directly to knowledge on: the distribution and nature of dark matter; the processes of star formation; and the origin and growth of large-scale structure. Extremely low-luminosity dwarfs are only detectable at very short distances, within or near the Local Group, so very few are known. The first part (southern hemisphere) of an all-sky survey to discover more has resulted in one certain and one borderline new Local Group dwarf, plus a number of more distant dwarfs and low surface brightness galaxies. Extending this survey to the northern hemisphere, we have produced a list of approximately one hundred dwarf galaxy candidates. We propose to continue (and, if possible, complete) follow-up imaging of these to determine their nature.
Hau George
Irwin Mike
Whiting Alan
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