GAMA blue spheroids within 87 Mpc

DOI

In this paper, we test if nearby blue spheroid (BSph) galaxies may become the progenitors of star-forming spiral galaxies or passively evolving elliptical galaxies. Our sample comprises 428 galaxies of various morphologies in the redshift range 0.002

Identifier
DOI http://doi.org/10.26093/cds/vizier.74750788
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/475/788
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/475/788
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/475/788
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/475/788
Provenance
Creator Mahajan S.; Drinkwater M.J.; Driver S.; Hopkins A.M.; Graham A.W.,Brough S.; Brown M.J.I.; Holwerda B.W.; Owers M.S.; Pimbblet K.A.
Publisher CDS
Publication Year 2021
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; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics