Spiral galaxies - Open Access .click

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Publications of the Astronomical Society of the Pacific, 1993
The global properties of galaxies such as their observed luminosities may be severely affected by internal obscuration of the stars by dust. In this thesis I examine the amount and extent of this obscuration using the following approaches: For a sample of eight galaxies for which I have obtained multi-waveband optical and near-infrared observations I ...
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Phenomenology of Spiral Galaxies

1975
Galaxies have probably been formed from fluctuations in density and motion in the universe. Many cosmologists have suggested that the separation into individual units took place around the time of decoupling of matter and radiation, when the radius of the universe was about 1/1000th of the present radius.
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A population of red candidate massive galaxies ~600 Myr after the Big Bang

Nature, 2023
Pieter van Dokkum, Erica Nelson, Rachel Bezanson +2 more
exaly

Simulations of the formation, evolution and clustering of galaxies and quasars

Nature, 2005
Volker Springel, Simon D M White, Adrian Jenkins +2 more
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Properties of galaxies reproduced by a hydrodynamic simulation

Nature, 2014
Mark Vogelsberger, Shy Genel, Volker Springel +2 more
exaly

Cosmology and fundamental physics with the Euclid satellite

Living Reviews in Relativity, 2018
Luca Amendola +2 more
exaly

High molecular gas fractions in normal massive star-forming galaxies in the young Universe

Nature, 2010
Linda Tacconi, Reinhard Genzel, Alberto Bolatto +2 more
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Cosmology and Fundamental Physics with the Euclid Satellite

Living Reviews in Relativity, 2013
Luca Amendola, Stephen Appleby, Tessa Baker +2 more
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