Volume 511, February 2010
|Number of page(s)||4|
|Published online||26 February 2010|
Letter to the Editor
A coincidence between a hydrocarbon plasma absorption spectrum and the λ5450 DIB
Raymond and Beverly Sackler Laboratory for Astrophysics,
Leiden Observatory, Leiden University, PO Box 9513, 2300 RA
Leiden, The Netherlands e-mail: email@example.com
2 Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, The Netherlands
3 Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200B, 3000 Leuven, Belgium
4 Physics and Astronomy Department, University of British Columbia, Vancouver, BC V6T 1Z4, Canada
5 National Research Council of Canada, Herzberg Institute of Astrophysics, 5071 W. Saanich Road, Victoria, BC V9E 2E7, Canada
6 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
7 Department of Chemistry, University of Basel, Klingelbergstrasse 80, 4056 Basel, Switzerland
Accepted: 4 February 2010
Aims. The aim of this work is to link the broad λ5450 diffuse interstellar band (DIB) to a laboratory spectrum recorded through expanding acetylene plasma.
Methods. Cavity ring-down direct absorption spectra and astronomical observations of HD 183143 with the HERMES spectrograph on the Mercator Telescope on La Palma and the McKellar spectrograph on the DAO 1.2 m Telescope are compared.
Results. In the 543–547 nm region a broad band is measured with a band maximum at 545 nm and FWHM of 1.03(0.1) nm coinciding with a well-known diffuse interstellar band at λ5450 with an FWHM of 0.953 nm.
Conclusions. A coincidence is found between the laboratory and the two independent observational studies obtained at higher spectral resolution. This result is important, as a match between a laboratory spectrum and a – potentially lifetime broadened – DIB is found. A series of additional experiments were performed in order to unambiguously identify the laboratory carrier of this band, but this was not successful. The laboratory results, however, restrict the carrier to a molecular transient, consisting of carbon and hydrogen.
Key words: astrochemistry / techniques: spectroscopic / ISM: molecules / ISM: lines and bands
© ESO, 2010
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