Investigating the transport of angular momentum from young stellar objects

2008/02/16 by A. Chrysostomou, F. Bacciotti, B. Nisni +6 · 1 citation
Chemistry · Physics and Astronomy · #Astrophysics and Star Formation Studies #Molecular Spectroscopy and Structure #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078494

11 pages, 5 figures, accepted for publication in Astronomy & Astrophysics

arxiv created 2008/02/16 · openalex publication_date 2008/02/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

Aims. In this pilot study, we examine molecular jets from the embedded Class I sources, HH 26 and HH 72, to search, for the first time, for kinematic signatures of jet rotation from young embedded sources.

Citations

• Rotation of Jets from Young Stars: New Clues from theHubble Space TelescopeImaging Spectrograph
• Interaction of young stellar object jets with their accretion disk
• Accretion and ejection properties of embedded protostars: the case of HH26, HH34, and HH46 IRS

Cited by

• Electrostatic ion perturbations in kinematically complex shear flows