ISO LWS Spectroscopy of NGC 4945

Astronomy and Astrophysics – Astronomy

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Scientific paper

We have obtained fully sampled, low resolution (R=lambda / triangle lambda ~ 200) far-infrared (FIR) 42-197 mu m spectra of the southern AGN/starburst SB(s)cd galaxy NGC 4945 with the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO). The galaxy was observed at a central, NE, and SW position, each separated by 165'' with the instrument's ~ 75" aperture. The forbidden fine-structure transitions of [CII] 158 mu m and [OI] 63 mu m lines were detected at each position. Detections of the [OI] 145 mu m and [OIII] 88 mu m lines were also obtained at some positions. Using these lines and the total FIR continuum flux, we have modeled the properties of the warm atomic gas with photodissociation region (PDR) models (Tielens and Hollenbach, 1985; Wolfire et al. 1990; Kaufman et al. 1998). The low-J rotational transitions of OH at 53 mu m and 119 mu m are seen in absorption at the nuclear position. The total OH column density and the role of these lines in the pumping of the OH radio maser are considered for these two transitions. The NE and SW positions lie on the massive molecular ring. The ring versus the nuclear conditions are analyzed by comparing the CII/OI, CII/CO, and (CII+OI)/FIR ratios.

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