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Visiting non-Newtonian MOND gravity in low-mass galaxies
Uppsala University.
Uppsala University.
1999 (English)In: ASTRONOMY AND ASTROPHYSICS, ISSN 0004-6361, Vol. 345, no 1, p. 36-42Article in journal (Other scientific) Published
Abstract [en]

The consistency of the application of Milgrom's modified dynamics (MOND) is tested in low-mass disc galaxies. If the existing Toomre parameter is a good indicator of axisymmetric instabilities, then catastrophic ring instabilities are predicted to occur i

Place, publisher, year, edition, pages
SPRINGER VERLAG , 1999. Vol. 345, no 1, p. 36-42
Keywords [en]
gravitation; galaxies : individual : IC 2574; galaxies : individual : NGC 1560; galaxies : irregular; galaxies : kinematics and dynamics; cosmology : dark matter; SURFACE BRIGHTNESS GALAXIES; EXTENDED ROTATION CURVES; DARK-MATTER HYPOTHESIS; H-II REGIONS;
Identifiers
URN: urn:nbn:se:uu:diva-85280OAI: oai:DiVA.org:uu-85280DiVA, id: diva2:113188
Note
Addresses: Sanchez-Salcedo FJ, Univ Newcastle Upon Tyne, Dept Math, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England. Univ Newcastle Upon Tyne, Dept Math, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England. Astron Observ, S-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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