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Distribution of dust clouds around the central engine of NGC 1068
Daigo Tomono, Hiroshi Terada, Naoto Kobayashi
We studied the distribution of dust clouds around the central engine of NGC 1068 based on shifted-and-added 8.8 - 12.3 micron (MIR) multi-filter images and 3.0 - 3.9 micron (L-band…
Large Silicon Abundance in Photodissociation Regions
Yoko Okada, Takashi Onaka, Takao Nakagawa +3
We have made one-dimensional raster-scan observations of the rho Oph and sigma Sco star-forming regions with two spectrometers (SWS and LWS) on board the ISO. In the rho Oph region…
Mid Infrared Spectral Energy Distribution of NGC 1068 with 0.1 arcsec Spatial Resolution
Daigo Tomono, Yoshiyuki Doi, Tomonori Usuda +1
The central region of the Seyfert 2 galaxy NGC 1068 is imaged in the mid infrared (MIR) using the Mid-Infrared Test Observation System on the 8.2 m Subaru Telescope. The oversampli…