Kinematics of YSO Molecular Hydrogen Outflows

Details Kinematics of YSO Molecular Hydrogen Outflows Kinematics of YSO Molecular Hydrogen Outflows

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..13...94s&link_type=abstract

Emission Lines from Jet Flows, Isla Mujeres, Q.R., México, November 13-17, 2000 (Eds. W. J. Henney, W. Steffen, A. C. Raga, and

Astronomy and Astrophysics

Astronomy

1

Ism: Jets And Outflows, Ism: Kinematics And Dynamics, Ism: Molecules, Stars: Formation

Scientific paper

As part of an on-going kinematical survey of molecular outflows, we describe observations of the 2.12 mu m line of H[2] for objects such as OMC-1, HH 211, HH 212, DR 21, Ceph A and S187-IR . The observations were made with the CAMILA IR-camera and an imaging Fabry-Pérot etalon at the 2.12 m telescope of the Observatorio Astronómico Nacional in San Pedro Mártir. A 22 km s-1 (FWHM) resolution allows us to determine the global kinematics of these sources. We show that many of them are consistent with theoretical models such as the jet driven molecular outflow paradigm. A flux versus velocity relation, similar to the one observed for CO outflows, is revealed by H[2] velocity structure.

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