Young T Tauri star in CB 26 molecular outflows Virtual Observatory Resource

Authors

1. Launhardt R.
2. Pavlyuchenkov Ya.
3. Gueth F.
4. Chen X.
5. Dutery A.,Guilloteau S.
6. Henning T.
7. Pietu V.
8. Schreyer K.
9. Semenov D.

Published by

CDS

Abstract

The disk-outflow connection is thought to play a key role in extracting excess angular momentum from a forming proto-star. Although jet rotation has been observed in a few objects, no rotation of molecular outflows has been unambiguously reported so far. We report new millimeter-interferometric observations of the edge-on T-Tauri-star - disk system in the isolated Bok globule CB-26. The aim of these observations was to study the disk-outflow relation in this 1Myr old low-mass young stellar object.

Keywords

1. molecular-clouds
2. pre-main-sequence-stars

Bibliographic source Bibcode

2009A&A...494..147L

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/494/147

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/494/147

Document Object Identifer DOI

doi:10.26093/cds/vizier.34940147

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http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/494/147

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