Investigating the transport of angular momentum from young stellar objects
A. ChrysostomouCentre for Astrophysics Research, Science & Technology Research Institute, University of Hertfordshire, Hatfield, AL10 9AB, UK e-mail: [email protected]F. BacciottiINAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125, Florence, ItalyB. NisiniINAF – Osservatorio Astronomico di Roma, via di Frascati 33, 00040 Monte Porzio Catone, ItalyT. P. RaySchool of Cosmic Physics, Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, IrelandJ. EislöffelThüringer Landessternwarte, Sternwarte 5, 07778 Tautenberg, GermanyC. J. DavisJoint Astronomy Centre, 660 N. A'ohoku Place, Hilo, Hawaii 96720, USAM. Takami
2008en
ABI
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.
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