Abstract
Maps of selected transitions in the nuclear region of the galaxy IC 342
are presented. The observations were taken with the IRAM 30 m telescope.
It is shown that molecular gas in the nucleus is warm and that physical
conditions vary with position in the galaxy. Far infrared measurement of
the OI 63 micron fine structure line indicate that the atomic and
molecular gas pressures are both equal to 300,000/cc/K, 10 times larger
than in our Galaxy.
Original language | English |
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Pages (from-to) | 589 |
Journal | Highlights of Astronomy |
Volume | 8 |
Publication status | Published - 1-Feb-1989 |
Keywords
- Density (Number/Volume)
- Galactic Nuclei
- Infrared Astronomy
- Molecular Spectra
- Mapping
- Milky Way Galaxy
- Molecular Clouds