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The Galaxy platform for accessible, reproducible and collaborative biomedical analyses: 2022 update

Nucleic Acids Research, 2022
Galaxy is a mature, browser accessible workbench for scientific computing. It enables scientists to share, analyze and visualize their own data, with minimal technical impediments.
Anup Kumar, Dave Clements, Frederik Coppens   +2 more
exaly   +2 more sources

The Galaxy in Context: Structural, Kinematic, and Integrated Properties [PDF]

Annual Review of Astronomy and Astrophysics, 2016
Our Galaxy, the Milky Way, is a benchmark for understanding disk galaxies. It is the only galaxy whose formation history can be studied using the full distribution of stars from faint dwarfs to supergiants.
Joss Bland-Hawthorn, Ortwin Gerhard
exaly   +2 more sources

The Galaxy platform for accessible, reproducible and collaborative biomedical analyses: 2018 update

Nucleic Acids Research, 2018
Galaxy (homepage: https://galaxyproject.org, main public server: https://usegalaxy.org) is a web-based scientific analysis platform used by tens of thousands of scientists across the world to analyze large biomedical datasets such as those found in ...
Enis Afgan, Dannon Baker, Bérénice Batut   +2 more
exaly   +2 more sources

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A repeating fast radio burst source localized to a nearby spiral galaxy

Nature, 2020
Fast radio bursts (FRBs) are brief, bright, extragalactic radio flashes1,2. Their physical origin remains unknown, but dozens of possible models have been postulated3. Some FRB sources exhibit repeat bursts4–7.
Benito Marcote, Kenzie Nimmo, Jason Hessels   +2 more
exaly   +2 more sources

Galaxies and Clusters of Galaxies [PDF]

, 2002
The leap into deep space outside our Milky Way Galaxy, into the realm of the distant galaxies (or the extragalactic nebulae, as they were formerly called), and the beginnings of a cosmology based on observations, will be considered throughout history to be one of the most important achievements of the 20th century.
Bodo Baschek, Albrecht Unsöld
openaire   +1 more source

Galaxies and Clusters of Galaxies

1987
Numerous galaxies similar to our own can be observed at distances far beyond the boundaries of our Galaxy. Sometimes they are referred to as “extragalactic nebulae” because they look like faint nebulae when seen through small telescopes. Consequently they were initially given names such as the “Magellanic Clouds”, the “Andromeda nebula” and so forth.
Georgios Contopoulos, Dimitrios Kotsakis
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Galaxies and Galaxy Groups

2000
Before stellar evolution theory reached its present stage, galactic evolution ideas were tentative and depended not so much on physical arguments (e.g. galactic dynamics) but intuitive notions based on observations of galaxy shapes. Historically this is quite understandable.
Michael Stecker, Bernard Abrams
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The Origin of Galaxies and Clusters of Galaxies

Science, 1984
Debate on how galaxies and clusters of galaxies formed has reached an interesting stage at which one can find arguments for quite different scenarios. The galaxy distribution has a complex "frothy" character that could be the fossil of a network of protoclusters or pancakes that produced galaxies.
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Galaxies and Galaxy Groups

2004
Few galaxies are loners: almost all are members of groups of at least a dozen systems. The Milky Way is no exception. It is the second brightest in a group of three dozen, mostly dwarf, galaxies. The brightest member of the Local Galaxy Group is the Andromeda Spiral M31. The most luminous members of the Local Group, including all those visible with any
Craig Crossen, Gerald Rhemann
openaire   +2 more sources