A near-infrared Fabry-Perot imager at CRL 1.5m telescope and the structure and velocity field of shocked H2 emission in Orion KL region

Details A near-infrared Fabry-Perot imager at CRL 1.5m telescope and the structure and velocity field of shocked H2 emission in Orion KL region A near-infrared Fabry-Perot imager at CRL 1.5m telescope and the structure and velocity field of shocked H2 emission in Orion KL region

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994exa.....3..315s&link_type=abstract

Experimental Astronomy, vol. 3, no. 1-4, p. 315-316

Astronomy and Astrophysics

Astronomy

Etalons, Fabry-Perot Interferometers, Infrared Astronomy, Infrared Telescopes, Near Infrared Radiation, Orion Nebula, Pre-Main Sequence Stars, Astronomical Maps, Molecular Clouds

Scientific paper

We have developed a near-infrared Fabry-Perot imager at the Nasmyth
focus of the Communications Research Laboratory (CRL) 1.5 m telescope at
Tokyo. Using this wide field Fabry-Perot imager, we obtained
continuum-subtracted images of the H2 upsilon = 1 - 0 S(1) line for the
Orion KL region.

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