Results 271 to 280 of about 30,270 (299)
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Populations In Local Group Galaxies
Annual Review of Astronomy and Astrophysics, 1989developed primarily by W. Baade in the 1950s, was inspired by the apparent dichotomy of galaxy content. Some galaxies (spirals and irregulars) seemed to be made up largely of bright, blue stars, with an admixture of interstellar material, whereas others (ellipticals) seemed to be made up exclusively offaint red stars (13). Baade called the two kinds of
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Simulation of Compact Groups of Galaxies
Astrophysics and Space Science, 1986Self-consistent simulations of seven groups of galaxies with halos have been performed to find a constraint upon the size of missing halos around spiral galaxies. An initial galaxy, which consists of 100 superstars, has half-mass radius 41 kpc and central velocity dispersion 235 km s−1. The simulations start from the epoch of maximum expansion.
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Active galaxies in groups of galaxies
Astrophysics, 1982G. M. Tovmasyan, �. Ts. Shakhbazyan
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Chemodynamical models of our Galaxy
Monthly Notices of the Royal Astronomical Society, 2023James Binney +2 more
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The Galaxy in Context: Structural, Kinematic, and Integrated Properties
Annual Review of Astronomy and Astrophysics, 2016Joss Bland-Hawthorn, Ortwin Gerhard
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Faint galaxies in groups of bright galaxies
Astrophysics, 1991A. T. Kalloglyan, S. R. Unanyan
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The Evolution of Galaxy Structure Over Cosmic Time
Annual Review of Astronomy and Astrophysics, 2014Christopher Conselice
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Physical Models of Galaxy Formation in a Cosmological Framework
Annual Review of Astronomy and Astrophysics, 2015Romeel Dave
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