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A&A 484, L43-L46 (2008)
DOI: 10.1051/0004-6361:200809985
Letter
6.7 GHz methanol absorption toward the Seyfert 2 galaxy NGC 3079
C. M. V. Impellizzeri, C. Henkel, A. L. Roy, and K. M. MentenMax-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
e-mail: violette@mpifr-bonn.mpg.de
Received 16 April 2008 / Accepted 2 May 2008
Abstract
The detection of the 6.7 GHz line of methanol (CH3OH) is reported
for the first time toward an object beyond the Magellanic
Clouds. Using the Effelsberg 100 m telescope, two absorption features
were identified toward the Seyfert 2 galaxy NGC 3079. Both components
probably originated on lines-of-sight toward the central region,
presumably absorbing the radio continuum of the nuclear sources A, B,
and E of NGC 3079. One absorption feature, at the systemic velocity,
is narrow and may arise from gas not related to the nuclear
environment of the galaxy. The weaker blue-shifted component is wider
and may trace outflowing gas. Total A-type CH3OH column densities
are estimated to be between a few times 1013 and a few times
1015 cm-2. Because of a highly frequency-dependent
continuum background, the overall similarity of HI, OH, and
CH3OH absorption profiles hints at molecular clouds that cover the
entire area occupied by the nuclear radio continuum sources
(~4 pc).
Key words: galaxies: Seyfert -- galaxies: nuclei -- galaxies: starburst -- galaxies: active -- galaxies: individual: NGC 3079 -- radio lines: galaxies
© ESO 2008
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