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相关论文: Interpretation of the Tadpole VV29 Merging Galaxy …

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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…

天体物理学 · 物理学 2008-04-01 Carl H. Gibson

Hubble Space Telescope images of the Helix Planetary Nebula are interpreted using the hydro-gravitational-dynamics theory (HGD) of Gibson 1996-2006. HGD claims that baryonic-dark-matter (BDM) dominates the halo masses of galaxies (Schild…

天体物理学 · 物理学 2007-11-02 Carl H. Gibson , Rudolph E. Schild

Self-gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the…

天体物理学 · 物理学 2008-08-26 Carl H. Gibson , Rudolph E. Schild

Wide angle Hubble Space Telescope (HST/ACS) images of the Helix Planetary Nebula (NGC 7293) are interpreted using the hydro-gravitational theory (HGT) of Gibson 1996-2000 that predicts the baryonic dark matter and interstellar medium (ISM)…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson , Rudolph E. Schild

Tadpole galaxies have a head-tail shape with a large clump of star formation at the head and a diffuse tail or streak of stars off to one side. We measured the head and tail masses, ages, surface brightnesses, and sizes for 66 tadpoles in…

宇宙学与河外天体物理 · 物理学 2015-05-19 Bruce G. Elmegreen , Debra Meloy Elmegreen

The gravitational hydrodynamics of the primordial plasma with neutrino hot dark matter is considered as a challenge to the bottom-up cold dark matter paradigm. Viscosity and turbulence induce a top-down fragmentation scenario before and at…

宇宙学与河外天体物理 · 物理学 2009-12-08 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudy E. Schild

Within the GAs Stripping Phenomena in galaxies with MUSE (GASP) sample, we identified an ongoing 1:1 merger between two galaxies and the consequent formation of a tidal dwarf galaxy (TDG). The system is observed at z = 0.05043 and is part…

In the Hubble Ultra Deep Field (HUDF) an abundance of galaxies is seen with a knot at one end plus an extended tail, resembling a tadpole. These "tadpole galaxies" appear dynamically unrelaxed--presumably in an early merging state--where…

天体物理学 · 物理学 2009-11-13 A. N. Straughn , S. H. Cohen , R. E. Ryan , N. P. Hathi , R. A. Windhorst , R. A. Jansen

The Galactic halo is supposed to form from merging with nearby dwarf galaxies. In order to probe different components of the Galactic halo, we have applied the Gaussian Mixture Models method to a selected sample of metal poor stars with…

星系天体物理 · 物理学 2021-06-23 Xilong Liang , Yuqin Chen , Jingkun Zhao , Gang Zhao

The first structures were proto-voids formed in the primordial plasma. Viscous and weak turbulence forces balanced gravitational forces when the scale of causal connection at time 30,000 years matched the viscous and turbulent Schwarz…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson

Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the…

天体物理学 · 物理学 2008-04-01 Carl H. Gibson , Rudolph E. Schild

Observations of the interstellar medium by the Herschel, Planck etc. infrared satellites throw doubt on standard {\Lambda}CDMHC cosmological processes to form gravitational structures. According to the Hydro-Gravitational-Dynamics (HGD)…

综合物理 · 物理学 2012-11-06 Carl H. Gibson

Westerbork Radio Synthesis Telescope observation of the galaxy VV29=Arp188=UGC10214 shows that there are at least three distinct dynamical components whose kinematics can be traced in 21cm line emission. The system appears to be the result…

天体物理学 · 物理学 2009-11-07 F. H. Briggs , O. Moller , J. L. Higdon , N. Trentham , E. Ramirez-Ruiz

Tadpole galaxies are metal-poor dwarfs with typically one dominant star-forming region, giving them a head-tail structure when inclined. A metallicity drop in the head suggests that gas accretion with even lower metallicity stimulated the…

Observations are compared to conflicting predictions about self-gravitational structure formation by the hydro-gravitational theory (HGT) of Gibson 1996-2003 versus cold-dark-matter hierarchical-clustering-cosmology (CDMHCC) and the Jeans…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson , Rudy Schild

[abridged] Aims. We observed the outer parts of NGC 1569 and NGC 4449, two of the closest and strongest dwarf starburst galaxies in the local universe, to characterize their stellar density and populations, and obtain new insights into the…

宇宙学与河外天体物理 · 物理学 2015-05-27 Agnieszka Ryś , Aaron J. Grocholski , Roeland P. van der Marel , Alessandra Aloisi , Francesca Annibali

A clear link between a dwarf-dwarf merger event and enhanced star formation (SF) in the recent past was recently identified in the gas-dominated merger remnant VCC 848, offering by far the clearest view of a gas-rich late-stage dwarf-dwarf…

Gravitational hydrodynamics acknowledges that hydrodynamics is essentially nonlinear and viscous. In the plasma, at $z=5100$, the viscous length enters the horizon and causes fragmentation into plasma clumps surrounded by voids. The latter…

宇宙学与河外天体物理 · 物理学 2010-03-03 Theo M. Nieuwenhuizen , Carl H. Gibson , Rudolph E. Schild

Mergers between red galaxies are observed to be common in the nearby Universe, and are thought to be the dominant mechanism by which massive galaxies grow their mass at late times. These ``dry'' mergers can be readily identified in very…

天体物理学 · 物理学 2009-11-13 K. E. Whitaker , P. G. van Dokkum

The physical mechanisms driving star formation (SF) in galaxies are still not fully understood. Tidal dwarf galaxies (TDGs), made of gas ejected during galaxy interactions, seem to be devoid of dark matter and have a near-solar metallicity.…

星系天体物理 · 物理学 2016-05-25 U. Lisenfeld , J. Braine , P. A. Duc , M. Boquien , E. Brinks , F. Bournaud , F. Lelli , V. Charmandaris
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