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Simulation of Compact Groups of Galaxies

Astrophysics and Space Science, 1986
Self-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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Populations In Local Group Galaxies

Annual Review of Astronomy and Astrophysics, 1989
developed 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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Active galaxies in groups of galaxies

Astrophysics, 1982
G. M. Tovmasyan, �. Ts. Shakhbazyan
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Galaxy Groups

Astronomische Nachrichten, 2003
Ralf-Jürgen Dettmar, Volker Müller
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A Population of Red Candidate Massive Galaxies ~600 Myr After the Big Bang

Nature, 2023
Rachel Bezanson   +2 more
exaly  

A Massive Quiescent Galaxy at Redshift 4.658

Nature, 2023
Daniel Magee   +2 more
exaly  

Faint galaxies in groups of bright galaxies

Astrophysics, 1991
A. T. Kalloglyan, S. R. Unanyan
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Systematic Variation of the Stellar Initial Mass Function in Early-Type Galaxies

Nature, 2012
Paolo Serra   +2 more
exaly  

Galaxies at Redshifts 5 to 6 With Systematically Low Dust Content and High [C Ii] Emission

Nature, 2015
Gareth C. Jones   +2 more
exaly  

Rapidly Star-Forming Galaxies Adjacent to Quasars at Redshifts Exceeding 6

Nature, 2017
Roberto Decarli   +2 more
exaly  

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