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Modified Newtonian Dynamics Rotation Curves of Very Low Mass Spiral Galaxies

  • Milgrom M
  • Sanders R
The Astrophysical Journal (2007) 658(1) L17-L20
DOI: 10.1086/513695
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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.

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CITATION STYLE

APA

Milgrom, M., & Sanders, R. H. (2007). Modified Newtonian Dynamics Rotation Curves of Very Low Mass Spiral Galaxies. The Astrophysical Journal, 658(1), L17–L20. https://doi.org/10.1086/513695

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