TY - JOUR
T1 - Visiting non-Newtonian MOND gravity in low-mass galaxies
AU - Sánchez-Salcedo, F. J.
AU - Hidalgo-Gámez, A. M.
PY - 1999
Y1 - 1999
N2 - 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 in the gas component of dwarf gas-rich galaxies. These dynamical instabilités would promote large gas concentrations and would destroy the smoothness of the disc in a few orbit times. As a rule, the attributed property of MOND to explain that the observed rotation curve is a scaled version of the rotation curve derived from the HI alone, may break down. Decreasing the adopted distance to these galaxies in order to recover gas stability is unsatisfactory. These points are illustrated with the low-mass galaxies IC 2574 and NGC 1560, and with the tidal tail in the interacting galaxies NGC 4485/4490.
AB - 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 in the gas component of dwarf gas-rich galaxies. These dynamical instabilités would promote large gas concentrations and would destroy the smoothness of the disc in a few orbit times. As a rule, the attributed property of MOND to explain that the observed rotation curve is a scaled version of the rotation curve derived from the HI alone, may break down. Decreasing the adopted distance to these galaxies in order to recover gas stability is unsatisfactory. These points are illustrated with the low-mass galaxies IC 2574 and NGC 1560, and with the tidal tail in the interacting galaxies NGC 4485/4490.
KW - Cosmology: dark matter
KW - Galaxies: individual: IC 2574
KW - Galaxies: individual: NGC 1560
KW - Galaxies: irregular
KW - Galaxies: kinematics and dynamics
KW - Gravitation
UR - http://www.scopus.com/inward/record.url?scp=0009955103&partnerID=8YFLogxK
M3 - Artículo
SN - 0004-6361
VL - 345
SP - 36
EP - 42
JO - Astronomy and Astrophysics
JF - Astronomy and Astrophysics
IS - 1
ER -