Sub-mm images of SSTB213 J041757.75+274105.5

DOI

We observed the proto brown dwarf candidate SSTB213 J041757 with the Submillimeter Array to search for CO molecular outflow emission from the source. Our CO maps do not show any outflow emission from the proto brown dwarf candidate. The non-detection implies that the molecular outflows from the source are weak; deeper observations are therefore needed to probe the outflows from the source.

Cone search capability for table J/A+A/564/A32/list (List of FITS data cube)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35640032
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/564/A32
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/564/A32
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/564/A32
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/564/A32
Provenance
Creator Phan-Bao N.; Lee C.-F.; Ho P.T.P.; Martin E.L.
Publisher CDS
Publication Year 2014
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; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy