MOND rotation curves of very low mass spiral galaxies

Abstract

We present MOND analysis for several of the lowest mass disc galaxies currently amenable to such analysis--with (baryonic) masses below 4x10^8 solar masses. The agreement is good, extending the validity of MOND and its predicted mass velocity relation, to such low masses.

8 pages, 1 figure

References in corpus (1)

• NGC 3741: dark halo profile from the most extended rotation curve

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