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Evolution of Galaxies

1976
Galaxies come in a wide variety of shapes and sizes. Until now, it has not really mattered for the purposes of this book just how galaxies differ from one another — we have been primarily concerned to account for their existence, and have considered them as ‘test particles’ which enable us to observe the expansion of the Universe. But if we are to find
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Galaxy Evolution

Astronomische Nachrichten, 2003
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Galaxies and their Evolution

1975
The methods by which the masses and mass-to light ratios of galaxies are determined from the velocity dispersions of stars and from dynamical studies of clusters of galaxies are outlined. It is concluded that while small clusters give no evidence for “missing mass” there is a discrepancy of about a factor of 5 in the case of large clusters.
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The role of submillimetre galaxies in galaxy evolution

2011
This thesis presents a comprehensive study of high redshift submillimetre galaxies (SMGs) using the deepest multi-wavelength observations. The submm sample consists of galaxies detected at 850 μm with the Submillimetre Common User Bolometer Array (SCUBA) in the Great Observatories Origins Deep Survey-North region. Using the deep Spitzer Space Telescope
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Galaxy Evolution

Annals of the New York Academy of Sciences, 1993
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Exploring the Sun’s birth radius and the distribution of planet building blocks in the Milky Way galaxy: a multizone Galactic chemical evolution approach

Monthly Notices of the Royal Astronomical Society, 2023
Junichi Baba   +2 more
exaly  

The Evolution of Galaxy Structure Over Cosmic Time

Annual Review of Astronomy and Astrophysics, 2014
Christopher J Conselice
exaly  

Galaxy Evolution

Physics Essays, 1999
Frank M. Meno, Kassem Awada
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