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Galaxy Zoo: Bar Lengths in Nearby Disk Galaxies
Published 2011“…We present an analysis of bar length measurements of 3150 local galaxies in a volume limited sample of low redshift (z < 0.06) disk galaxies. …”
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Galaxy Zoo: Chiral correlation function of galaxy spins
Published 2008“…Galaxy Zoo is the first study of nearby galaxies that contains reliable information about the spiral sense of rotation of galaxy arms for a sizeable number of galaxies. …”
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Galaxy Zoo: bar lengths in local disc galaxies
Published 2011“…We present an analysis of bar length measurements of 3150 local galaxies in a volume-limited sample of low-redshift (z < 0.06) disc galaxies. …”
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The influence of redshift information on galaxy-galaxy lensing measurements
Published 2005Journal article -
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Galaxy Zoo: Bulgeless Galaxies With Growing Black Holes
Published 2012“…The growth of supermassive black holes appears to be driven by galaxy mergers, violent merger-free processes and/or `secular' processes. …”
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Galaxy Zoo: kinematics of strongly and weakly barred galaxies
Published 2023“…Our sample, which is divided between strongly and weakly barred galaxies identified via Galaxy Zoo, is the largest that this method has been applied to. …”
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Galaxy Zoo: The fraction of merging galaxies in the SDSS and their morphologies
Published 2010“…We present the largest, most homogeneous catalogue of merging galaxies in the nearby Universe obtained through the Galaxy Zoo project - an interface on the World Wide Web enabling large-scale morphological classification of galaxies through visual inspection of images from the Sloan Digital Sky Survey (SDSS). …”
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Charmed Galaxies
Published 2023-01-01“…First evidence for neutrino emission from the active galaxies TXS0506+056 and NGC1068 indicates that a significant fraction comes from such sources. …”
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Explosions in galaxies
Published 2002-12-01“…Large-scale vertical structures and outflows observed in galaxies are discussed in this context.…”
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Nomads of the Galaxy
Published 2012“…We estimate that there may be up to ∼10 5 compact objects in the mass range 10 -8-10 -2M ⊙ per-main-sequence star that are unbound to a host star in the Galaxy. We refer to these objects as nomads; in the literature a subset of these are sometimes called free-floating or rogue planets. …”
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Galaxy masses
Published 2014“…Galaxy masses play a fundamental role in our understanding of structure formation models. …”
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Accretion by Galaxies
Published 2000“…Both theory and observation indicate that galaxies like the Milky Way accrete matter at the rate of a few Msun per year.…”
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