Shocks and Star Formation in Orion: First Light with GriF

Details Shocks and Star Formation in Orion: First Light with GriF Shocks and Star Formation in Orion: First Light with GriF

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sao..conf..229g&link_type=abstract

Science with Adaptive Optics, Proceedings of the ESO Workshop Held at Garching, Germany, 16-19 September 2003. Edited by W. Bran

Physics

Optics

Scientific paper

A new instrument, GriF", has been used on the Canada-France-Hawaii Telescope to record spatially and velocity resolved images of the core of the Orion Molecular Cloud (OMC1). GriF combines Fabry-Perot interferometry with PUEO adaptive optics, [1]. Using the H2 v=1-0 S(1) line at 2.121μm, diffraction limited spatial resolution of 0.''15 and velocity discrimination as good as 1 kms-1 has been achieved in the brighter regions. This work is reported in detail in [2].

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