The Kinematics of Late-Type Low Surface Brightness Galaxies

Details The Kinematics of Late-Type Low Surface Brightness Galaxies The Kinematics of Late-Type Low Surface Brightness Galaxies

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aspc..182..373d&link_type=abstract

Galaxy Dynamics, proceedings of a conference held at Rutgers University, 8-12 Aug 1998. ASP Conference Series vol. 182 (San Fran

Computer Science

Scientific paper

I describe the dynamics of a sample of late-type low surface brightness
(LSB) galaxies, and show that these galaxies are completely dominated by
dark matter, even under the (dubious) assumption of maximum disk. I show
trends of halo parameters with surface brightness and conclude that LSB
galaxies probably inhabit low density halos.

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