Colours and HI line observations in Virgo

DOI

In order to investigate the nature of dwarf low surface brightness (LSB) galaxies we have undertaken a deep B- and I-band CCD survey of a 14-deg^2^ strip in the Virgo Cluster and applied a Fourier convolution technique to explore its dwarf galaxy population down to a central surface brightness of ~26Bmag/arcsec^2^ and a total absolute B magnitude of ~-10. In this paper we carry out an analysis of their morphology, (B-I) colours and atomic hydrogen content.

Cone search capability for table J/MNRAS/357/819/table3 (Objects not detected in H I at Arecibo)

Identifier
DOI http://doi.org/10.26093/cds/vizier.73570819
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/357/819
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/357/819
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/357/819
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/357/819
Provenance
Creator Sabatini S.; Davies J.; Van Driel W.; Baes M.; Roberts S.; Smith R.,Linder S.; O'neil K.
Publisher CDS
Publication Year 2006
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