Pitfalls in the identification of the 21 micron feature

Details Pitfalls in the identification of the 21 micron feature Pitfalls in the identification of the 21 micron feature

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..447a&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

2

Circumstellar Matter, Infrared Stars, Laboratory Methods

Scientific paper

The origin of the so-called "21 μm" feature that is especially prominent in the spectra of some carbon-rich protoplanetary nebulae is the matter of a lively debate. A large number of potential band carriers have been presented and discarded within the past decade. We present some of the problems related to the hitherto proposed feature identifications.

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