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Issue A&A
Volume 484, Number 3, June IV 2008
Page(s) L43 - L46
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:200809985
Published online 15 May 2008



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. Menten

Max-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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