Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
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Galaxy Zoo: CANDELS barred discs and bar fractionsGalaxy Zoo 2: detailed morphological classifications for 304 122 galaxies from the Sloan Digital Sky SurveyGalaxy Zoo: the dependence of the star formation–stellar mass relation on spiral disc morphologyGalaxy Zoo: secular evolution of barred galaxies from structural decomposition of multiband imagesGalaxy Zoo and sparcfire: constraints on spiral arm formation mechanisms from spiral arm number and pitch anglesGalaxy Zoo: finding offset discs and bars in SDSS galaxies★Galaxy Zoo: the interplay of quenching mechanisms in the group environmentGalaxy Zoo: star formation versus spiral arm numberGalaxy Zoo: comparing the demographics of spiral arm number and a new method for correcting redshift biasGalaxy Zoo: evidence for diverse star formation histories through the green valleyGalaxy Zoo: Mergers – Dynamical models of interacting galaxiesGalaxy Zoo: Are bars responsible for the feeding of active galactic nuclei at 0.2 < z < 1.0?The SAMI Galaxy Survey: asymmetry in gas kinematics and its links to stellar mass and star formation
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Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
description
article
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im Dezember 2012 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в грудні 2012
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name
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
@en
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
@nl
type
label
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
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Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
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prefLabel
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
@en
Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
@nl
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Galaxy Zoo: quantifying morphological indicators of galaxy interaction★
@en
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Kevin. R. V. Casteels
Ramin A. Skibba
William C. Keel
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P304
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10.1093/MNRAS/STS391
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P577
2012-12-06T00:00:00Z
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P819
2013MNRAS.429.1051C