Sub-mm images of SSTB213 J041757.75+274105.5 Virtual Observatory Resource

Authors

1. Phan-Bao N.
2. Lee C.-F.
3. Ho P.T.P.
4. Martin E.L.

Published by

CDS

Abstract

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.

Keywords

1. interstellar-medium
2. stellar-mass-loss
3. interferometry
4. protostars
5. radio-spectroscopy

Bibliographic source Bibcode

2014A&A...564A..32P

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ivo://CDS.VizieR/J/A+A/564/A32

Document Object Identifer DOI

doi:10.26093/cds/vizier.35640032

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