SECULAR EVOLUTION OF SPIRAL GALAXIES |
ZHANG XIAOLEI (US Naval Research Laboratory, Remote Sensing Division) |
1 | Zwaan, M.A., van der Hulst, J.M., de Blok, W.J.G., & Mc Gaugh, S.S. 1995, The Tully-Fisher relation for low surface brightness galaxies: implications for galaxy evolution, MNRAS, 273, L35 DOI |
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The centers of early-type galaxies with HST.Ⅳ. Central parameter relations
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On the influence of bars and star formation on galactic abundance gradients
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The Galaxy-Cluster-Supercluster connection
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Accretion discs in astrophysics
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The Tully-Fisher relation for low surface brightness galaxies: implications for galaxy evolution
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Secular evolution of spiral galaxies. I. A collective dissipation process
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The evolution of galaxies and stars
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Deciphering the last major invasion of the Milky Way
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Dynamics of galaxies in clusters
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Turbulence and star formation in molecular clouds
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The merging history of the Milky Way disk
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Evolution since Z=0.5 of the morphology-density relation for clusters of galaxies
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Line strength and line strength gradients in bulges along the Hubble sequence
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Observations of galaxy structure and dynamics
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Dissipation in barred galaxies -The growth of bulges and central mass concentration
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The cluster substructure-alignment correction
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Semianalytical models for the formation of disk galaxies. I. Constraints from the Tully-Fisher relation
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Probing high-reshift disks with damped Lya systems
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Galactic bulges
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Multiscaling of cosmic microwave background radiation
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Secular evolution of isolated barred galaxies. Ⅰ- Gravitational coupling between stellar bars and interstellar medium
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Dark matter and structure formation
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Kinematic misalignments in remnants of multiple mergers
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Galaxy formation through hierarchical clustering
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The arms of spiral galaxies
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Induced population gradients in galaxy merger remnants
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K giants and the total amount of matter near the sun
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Elliptical galaxies: Detailed structure, scaling relations and formation
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Rotation curves for spiral galaxies in clusters. I. - Data, global properties, and a comparison with field galaxies
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What amplifies the spirals
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The cosmic triangle: revealing the state of the universe
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Secular evolution of spiral galaxies. Ⅱ. Formation of quasi-stationary spiral modes
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CO (J=4-3) and [CI] observations of the Carina molecular cloud complex
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Evidence for a two-armed spiral in the Milky Way
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Large ground-based redshift surveys in the context of the HDF
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The cosmological constant and dark energy
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Box and peanut shapes generated by stellar bars
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The age of the solar neighborhood
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Galaxy number counts from the Sloan digital sky survey commissioning data
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Whirl theory of the origin of galaxies and clusters of galaxies
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On the generating mechanism of spiral structure
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The epochs of early-type galaxy formation
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New metallicity measurements of z¿3 Damped Lya systems
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A large scale energy source for feeding ISM turbulence in spiral galaxies
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Structure and evolution of long-lived spiral patterns in galaxies
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The Milky Way as a Galaxy
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Clusters of Galaxies in the SDSS
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Galaxy harassment and the evolution of clusters of galaxies
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The age of elliptical galaxies and bulges in a merger model
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Bar dissolution and bulge formation: and example of secular dynamical evolution in galaxies
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Evidence from the motions of old stars that the Galaxy collapsed
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The star formation history of the Milky Way
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Structure and dynamics of 3D N-body barred galaxies
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The formation of disk galaxies
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The alignment effect of brightest cluster galaxies in the SDSS
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Optical tracers of spiral wave resonances in galaxies. Ⅱ. Hidden three-arm spirals in a sample of 18 galaxies
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S0 and smooth-arm Sa's within the Hubble sequence
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Large-scale structure at z=1.2 outlined by Mg Ⅱ absorbers
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The evolution of galaxies in clusters. Ⅰ- ISIT photometry of C1 0024+1654 and 3C 295
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The age-velocity-dispersion relation in the solar neihborhood
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Evidence for secular evolution in late-type spirals
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NICMOS imaging of a cluster of extremely red galaxies at redshift z=2.38
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Secular evolution of isolated barred galaxies. Ⅱ. Coupling between stars and interstellar medium via star formation
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Cosmic turbulence and the angular momenta of astronomical systems
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Evolution and formation of early-types in clusters: Old disk galaxies
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The evolution of galaxies in clusters. Ⅱ- The galaxy content of nearby clusters
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The morphology of distant cluster galaxies. 1: HST observations of CL 0939+4713
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Faint blue galaxies
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Low surface brightness galaxies
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Nineteenth and twentieth century clouds over the twenty-first century virtual observatory
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The Kinematics of 3:1-merger remnants and the formation of low-luminosity elliptical galaxies
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High-resolution rotation curves of low surface brightness galaxies. Ⅱ. Mass models
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Maximum feedback and dark matter profiles of dwarf galaxies
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Dense stellar cores in merger remnants
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Secular evolution of spiral galaxies. Ⅲ. The Hubble sequence as a temporal evolution sequence
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Turbulent mixing, diffusion and gravity in the formation of cosmological structures: the fluid mechanics of dark matter
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Bar-halo interaction and bar growth
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Dissipative models of spiral galaxies
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Structure of merger remnants. Ⅴ. Kinematics
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Galaxy Alignment as a Probe of the Dynamical State of Clusters
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Dwarf galaxies in clusters
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Physical origin of galaxy scaling relations
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When did the large elliptical galaxies form?
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Morphological studies of the galaxy populations in distant 'Butcher-Oemler' clusters with HST. 1: AC 114 at Z=0.31 and Abell 370 at Z=0.37
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High resolution CO and HI observations of the interacting galaxy NGC 3627
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Quantitative Morphology and Color Gradient of E+A Galaxies in Distant Galaxy Clusters
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Are SA galaxies dark-matter poor?
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Flocculent and grant design spiral galaxies in groups - Time scales for the persistence of grand design spiral structures
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The Caltech faint galaxy redshift survey. ⅩⅥ. The Luminosity Function for Galaxies in the Region of the Hubble Deep Field-North to z=1.5
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Kinematics of extragalactic bulges: evidence that some bulges are really disks
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The evolution of disk galaxies in clusters
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Isophote shapes of elliptical galaxies. Ⅱ- Correlations with global optical, radio and X-ray properties
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Global properties of multiple merger remnants
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Radio astronomical in strumentation and obsrvations on Hat Creek Millimeter Interferometer
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Chemical and dynamical evolution of spiral galaxies
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Thin discs and dense bulges: what do they tell us about galaxies?
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The mass distribution in the galactic disc - Part two -Determination of the surface mass density of the galactic disc near the Sun
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The evolution of barred spiral galaxies in the Hubble Deep Fields North and South
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Chemo-spectrophotometric evolution of spiral galaxies. Ⅳ. Star formation efficiency and effective ages of spirals
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107 |
An outsider's view of the Galaxy - Photometric parameters, scale lengths, and absolute magnitudes of the spheroidal and disk components of our Galaxy
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108 |
Dark Halo and Disk Galaxy Scaling Laws in Hierarchical Universes
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Tidal triggering of Seyfert galaxies and quasars - Perturbed galaxy disk models versus observations
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110 |
On the infall of matter into clusters of galaxies and some effects on their evolution
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111 |
Gravitational collapse in dust lanes and the appearance of spiral structure in galaxies
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112 |
Stellar kinematics and interstellar turbulence
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Dynamics of superclusters as the most powerful test for theories of galaxy formation
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The diffusion of stellar orbits derived from the observed age-dependence of the velocity dispersion
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A large structure of galaxies at redshift Z approximately 3 and its cosmological implications
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