High resolution 1-20 micron imaging of the nuclear environment of NGC 1068

Details High resolution 1-20 micron imaging of the nuclear environment of NGC 1068 High resolution 1-20 micron imaging of the nuclear environment of NGC 1068

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..315c&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 315-316 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astronomy

1

Continuums, Emission Spectra, H Alpha Line, Imaging Techniques, Iron, Line Spectra, Narrowband, Near Infrared Radiation, Seyfert Galaxies, Astronomical Spectroscopy, Etalons, Fabry-Perot Interferometers, Imaging Spectrometers, Infrared Radiation

Scientific paper

We present new mid-infrared continuum and near-IR line images of the nuclear environment of the nearby (14 Mpc) Seyfert 2 galaxy NGC 1068. The 8, 10, and 19 micron data were measured with our new mid-IR array camera, MIRACLE, at UKIRT in Nov. 1991 while our images of the H2 2.121 micron and (Fe 2) 1.64 micron lines were obtained with FAST, the MPE imaging spectrometer, at the 4.2m William Herschel Telescope in Aug. 1991. The MIRACLE data were imaged through narrow band (lambda/delta(lambda) greater than or equal to 50) filters whereas FAST incorporates a Fabry-Perot etalon (lambda/delta(lambda) greater than or equal to 950).

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