Hydro-gravitational-dynamics interpretation of the tadpole VV29 merging galaxy system: BDM-halo star-cluster-wakes
Abstract
Hubble Space telescope (HST) images of merging galaxy system VV29 reveal the 0.3 Mpc baryonic-dark-matter (BDM) halo composed of primordial protoglobularstarcluster (PGC) clumps of planets. Star-cluster-wakes trace the merger by formation of stars from the planets. Aligned young globular star clusters (YGCs), star-wakes and dust-trails show the frictional, spiral passage of galaxy fragments VV29cdef in a long tail-like galaxy (VV29b) as the fragments merge on the accretion disk plane of the central spiral galaxy VV29a. The observations confirm the hydro-gravitational-dynamics (HGD) prediction of Gibson 1996 and quasar microlensing inference of Schild 1996 that the dark matter of galaxies is dominated by planets (PFPs) in million-solar-mass clumps. Globular star clusters (YGCs, OGCs, PGCs) preserve the density of the plasma epoch 30,000 years after the big bang when viscous supercluster-fragmentation began. Tadpole images show linear galaxy clusters reflecting turbulent vortex lines of protogalaxy fragmentation at the 0.003 Mpc Kolmogorov-Nomura scale of the plasma before transition to gas. The halo size indicates strong diffusion of PGC primordial-planet-clumps from a cooling protogalaxy as its planets freeze.
- Publication:
-
Problems of Practical Cosmology, Volume 1
- Pub Date:
- 2008
- DOI:
- 10.48550/arXiv.0803.4288
- arXiv:
- arXiv:0803.4288
- Bibcode:
- 2008pc1..conf..163G
- Keywords:
-
- Astrophysics
- E-Print:
- 8 pages, 7 figures, Practical Problems in Cosmology 2008, St. Petersburg RU, June 23-27