Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.GA 3representative citing papers
Bulge-disc decomposition on 2445 galaxies with I_E < 21 in Euclid ERO Perseus data shows B/T spanning 0-1, single-Sérsic radii as intermediates, and 0.3 mag median bulge-disc color differences driven by disc-dominated systems.
Visual inspection of CNN outputs from SDSS produces verified catalogues of 612 merging, 9372 irregular, 16822 edge-on, 575 dust-lane, 811 barred and 2150 ringed galaxies at 0.02<z<0.1 together with BPT-based nuclear activity types.
citing papers explorer
-
Tracing evolutionary pathways of bar-driven quenching in local Universe disc galaxies
Barred galaxies with residual central emission and NUV-r color transition at the bar end represent an intermediate evolutionary phase in bar-driven quenching before full central quenching.
-
Euclid: Galaxy morphology and photometry from bulge-disc decomposition of Early Release Observations
Bulge-disc decomposition on 2445 galaxies with I_E < 21 in Euclid ERO Perseus data shows B/T spanning 0-1, single-Sérsic radii as intermediates, and 0.3 mag median bulge-disc color differences driven by disc-dominated systems.
-
Machine learning technique for morphological classification of galaxies from SDSS. IV. Visual inspection vs CNN for merging, irregular, edge-on, barred, ringed, and with dust lanes galaxies at 0.02<z<0.1
Visual inspection of CNN outputs from SDSS produces verified catalogues of 612 merging, 9372 irregular, 16822 edge-on, 575 dust-lane, 811 barred and 2150 ringed galaxies at 0.02<z<0.1 together with BPT-based nuclear activity types.