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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

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Abstract

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 v=1−0 S(1) line for the Orion KL region.

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Sugai, H., Usuda, T., Kawabata, H. et al. 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. Exp Astron 3, 315–316 (1994). https://doi.org/10.1007/BF00430184

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Key words

  • Fabry-Perot imager
  • molecules
  • Orion Nebula
  • stars
  • pre-main-sequence