Parameter estimates for the orbits of M 32 and NGC 205 about the centre of mass of the M 31 system
The authors used simple kinematic, dynamic and geometrical assumptions to infer the orbital parameters of M32 and NGC 205 about M31. They find that both galaxies rotate in a retrograde sense compared to M31 indicating a possible common origin independent of the mother galaxy. Their periods, each ≅108yr, and their orbital radii, ≅12 kpc, are
Cepa, J. et al.
Fecha de publicación:
7
1988