Evolution of red spiral galaxies with GAMA

We use multiwavelength data from the Galaxy And Mass Assembly (GAMA) survey to explore the cause of red optical colours in nearby (0.002<z~47 per cent of all spirals in our sample. Furthermore, for a small subsample of our spiral galaxies that are detected in HI, we find that the SFR of gas-rich red spiral galaxies is lower by ~1dex than their blue counterparts.

Cone search capability for table J/MNRAS/491/398/table2 (The sky coordinates, z, (g-r) colour, ALFALFA ID and HI mass of spiral galaxies used in this work)

Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/491/398
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/491/398
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/491/398
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/491/398
Creator Mahajan S.; Gupta K.K.; Rana R.; Brown M.J.I.; Phillipps S.,Bland-Hawthorn J.; Bremer M.N.; Brough S.; Holwerda B.W.; Hopkins A.M.,Loveday J.; Pimbblet K.; Wang L.
Publisher CDS
Publication Year 2023
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics