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Investigating Dark Matter and MOND in Local Volume Galaxies

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Galaxies in the Local Volume

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP))

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Summary

Employing the most recent Local Volume Hi Survey (LVHIS) [5] data we are going to derive high-resolution Hi rotation curves for ~28 gas-rich nearby galaxies. Combining these kinematical results with stellar-mass tracing near-IR Hband photometry [5] and accurate TRGB distances [3, 4], we study the dark matter mass profiles of the sample galaxies and test the ability of Modified Newtonian Dynamics (MOND) to explain the observed rotation curves and to investigate the Mass Discrepancy-Acceleration Relation.

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Authors and Affiliations

  1. Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory, Cotter Rd, Weston, ACT 2611, Australia

    Nicolas J. Bonne

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  1. Nicolas J. Bonne
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Correspondence to Nicolas J. Bonne .

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    © 2008 Springer Science+Business Media B.V.

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    Bonne, N.J. (2008). Investigating Dark Matter and MOND in Local Volume Galaxies. In: Jerjen, H., Koribalski, B. (eds) Galaxies in the Local Volume. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-6933-8_8

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