Young T Tauri star in CB 26 molecular outflows

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34940147
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/494/147
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/494/147
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/494/147
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/494/147
Provenance
Creator Launhardt R.; Pavlyuchenkov Ya.; Gueth F.; Chen X.; Dutery A.,Guilloteau S.; Henning T.; Pietu V.; Schreyer K.; Semenov D.
Publisher CDS
Publication Year 2009
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; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy