Interpretation of the Stephan Quintet Galaxy Cluster using Hydro-Gravitational Theory
Stephan's Quintet (SQ) is a compact group of galaxies that has been well studied since its discovery in 1877 but
63 indexed results
Stephan's Quintet (SQ) is a compact group of galaxies that has been well studied since its discovery in 1877 but
Hubble Space Telescope (HST/ACS) images of the galaxy merger Tadpole are interpreted using the hydro-gravitational theory of Gibson 1996-2000 (HGT)
We examine the origin of heavy elements in the intracluster medium (ICM) of galaxy clusters, concentrating upon the roles played
The first results from the HI Parkes All-Sky Survey (HIPASS) provide a spectacular view of the global HI distribution in
We have examined the success rates of 19 American, Canadian, Australian, and Dutch graduate programs in producing astronomers. A 20-year
The fundamental tenet of the classical supernovae-driven wind model of elliptical galaxies is that the residual thermal energy of all
We revisit the problem of the flat slope of the Mg2 versus <Fe> relationship found for nuclei of elliptical galaxies
A quantum gravitational instability is identified at Planck scales between non-spinning extreme Schwarzschild black holes and spinning extreme Kerr black
We examine recent results of two kinds of microlensing experiments intended to detect galactic dark matter objects, and we suggest
We present preliminary results from a series of high-resolution N-body simulations that focus on 8 dark matter halos each of
Halo initial mass functions (IMFs) heavily biased toward white dwarf (WD) precursors ~1-8 Msun have been suggested as a suitable
Several speakers at IAU Symposium #187 (Cosmic Chemical Evolution) alluded to the zeroth-order agreement between Type II supernovae (SNe) stellar
A highly colloquialized summary of the Stromlo Workshop on High-Velocity Clouds, held Aug 14-15, 1998, at Mount Stromlo Observatory. The
The study of high-velocity clouds has progressed much since the appearance of the review article by Wakker & van Woerden
An overview of the 2001 astronomy job market is presented, highlighting the recent hiring trends which prospective PhD students and
We study the chemodynamical evolution of elliptical galaxies and their X-ray and optical properties using high-resolution cosmological simulations. Our Tree
A summary of recent Large Magellanic Cloud distance determinations mu(LMC) is presented, with an eye towards pinpointing the source(s) of
The enrichment of the intracluster medium (ICM) of galaxy clusters, within the framework of the supernovae-driven wind model for elliptical
Observations suggest that the structural parameters of disk galaxies have not changed greatly since redshift 1. We examine whether these
We describe the Anti-Grand Unification Model (AGUT) and the Multiple Point Principle (MPP) used to calculate the values of the
Chaotic, eddy-like motions dominated by inertial-vortex forces begin immediately at Planck scales in a hot big-bang cosmological model. This quantum-gravitational-dynamics
The first turbulent combustion arises in a hot big bang cosmological model Gibson (2004) where nonlinear exothermic turbulence permitted by
Jeans's (1902 & 1929) linear gravitational instability criterion gives truly spectacular errors in its predictions of cosmological structure formation according
The possibility of a gaseous halo stream which was stripped from the Sagittarius dwarf galaxy is presented. The total mass