Evolution of red spiral galaxies with GAMA

DOI

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)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74910398
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
Provenance
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>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics