A&A 412, L15-L18 (2003)
DOI: 10.1051/0004-6361:20031649
Letter
Interstellar SiN
P. Schilke1, S. Leurini1, K. M. Menten1 and J. Alcolea21 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
e-mail: [schilke,sleurini,kmenten]@mpifr-bonn.mpg.de
2 Observatorio Astronómico Nacional, C/Alfonso XII, 3, 28014 Madrid, Spain
e-mail: j.alcolea@oan.es
(Received 29 July 2003 / Accepted 23 October 2003)
Abstract
We report the detection of the silicon nitride (SiN)
N=2-1,
J=5/2-3/2 transition toward SgrB2(M), in absorption.
Although it has been seen in a circumstellar envelope before,
this is the first time this molecule has been detected in
interstellar space. We estimate a column density of
cm
-2, which is a factor of 20-50 lower than that of
silicon monoxide (SiO) toward this source. It is likely that
this molecule, like SiO and FeO, is created by gas-phase
chemistry after refractory elements, previously locked up in
grain cores, have been released by sputtering in shocks.
Key words: astrochemistry -- line: identification -- ISM: abundances -- ISM: molecules -- ISM: individual objects: SgrB2(M) -- radio lines: ISM
Offprint request: P. Schilke, schilke@mpifr-bonn.mpg.de
SIMBAD Objects
© ESO 2003

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