A new catalogue of bar lengths and widths from HST images of 8230 galaxies shows bars are about 13% weaker at higher redshift, with longer bars in higher-mass quiescent galaxies and trends consistent with slow quenching.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.GA 2years
2026 2roles
background 1polarities
background 1representative citing papers
Bars are transient secular features that track neither mass assembly nor speciation in the black hole-stellar mass plane, while S0 galaxies form via primeval transitions, faded spirals, and wet mergers, with dust attrition/retention and disc down-sizing sequences identified.
citing papers explorer
-
Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1
A new catalogue of bar lengths and widths from HST images of 8230 galaxies shows bars are about 13% weaker at higher redshift, with longer bars in higher-mass quiescent galaxies and trends consistent with slow quenching.
-
Clash of the Trident and Tuning Fork: insights from bar and spiral strength in the (massive black hole)-stellar mass diagrams, and the `Triangal' galaxy evolution schema
Bars are transient secular features that track neither mass assembly nor speciation in the black hole-stellar mass plane, while S0 galaxies form via primeval transitions, faded spirals, and wet mergers, with dust attrition/retention and disc down-sizing sequences identified.