Anomalously Excited OH and Competition between Maser Transitions toward Centaurus A

Details Anomalously Excited OH and Competition between Maser Transitions toward Centaurus A Anomalously Excited OH and Competition between Maser Transitions toward Centaurus A

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...448l.123v&link_type=abstract

Astrophysical Journal Letters v.448, p.L123

Astronomy and Astrophysics

Astronomy

33

Galaxies: Individual Name: Centaurus A, Galaxies: Nuclei, Ism: Molecules, Masers, Molecular Processes, Radio Lines: Galaxies

Scientific paper

The ground-state radio transitions of OH have been observed toward the nucleus of the nearby active galaxy Centaurus A, using the Australia Telescope Compact Array. The main lines at rest frequencies 1667 and 1665 MHz show molecular absorption at velocities similar to those observed for other molecular species at millimeter wavelengths, which indicates that the lines of sight at radio and millimeter wavelengths sample the same material. The satellite transitions at 1612 and 1720 MHz exhibit stimulated emission and absorption, including the first extragalactic detection of maser emission in the 1720 MHz line. A remarkable feature of the two satellite transitions is that they are conjugate for all velocity components, with one in emission and the other equally strong in absorption. This is explained as the competition of the two lines for the same inverting infrared radiation in the regime in which the infrared lines are just becoming optically thick. The transition from 1720 MHz to 1612 MHz maser emission depends critically on the OH column density and therefore yields direct information on the distribution of molecular gas.

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