Sequence Structure Emission in the Red Rectangle Bands

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© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation R. G. Sharp et al 2006 ApJ 639 194 DOI 10.1086/499260

0004-637X/639/1/194

Abstract

We report high-resolution (R ~ 37,000) integral field spectroscopy of the central region (r < 14'') of the Red Rectangle nebula surrounding HD 44179. The observations focus on the λ5800 emission feature, the bluest of the yellow/red emission bands in the Red Rectangle. We propose that the emission feature, widely believed to be a molecular emission band, is not a molecular rotation contour, but a vibrational contour caused by overlapping sequence bands from a molecule with an extended chromophore. We model the feature as arising in a polycyclic aromatic hydrocarbon (PAH) with 45-100 carbon atoms.

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10.1086/499260