Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus Conference proceedings 2001 Springer-Verlag Be

先鋒派

https://doi.org/10.1007/978-3-322-93659-2ment against the ‘maximum’ disk hypothesis. Next, density wave theory arguments are used to describe the morphology of the spiral arms of NGC 3223, 157, and 7083. It is shown that the ‘maximum’ disk hypothesis is not consistent with the observed morphologies of the galaxies.