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λ4430 Emission by Comet Hyakutake

Published online by Cambridge University Press:  21 February 2014

M. F. A'Hearn
Affiliation:
Department of Astronomy, University of Maryland College Park MD, 20742-2421, United States email: [email protected], [email protected]
D. D. Wellnitz
Affiliation:
Department of Astronomy, University of Maryland College Park MD, 20742-2421, United States email: [email protected], [email protected]
R. Meier
Affiliation:
Varian Medical Systems Imaging Laboratory GmbH, Täfernstrasse 7, CH5405, Baden-Dätwill, Switzerland email: [email protected]
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Abstract

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Comets provide a very different but well understood environment in which to search for DIBs. Observations of occultations by cometary comae have not detected DIBs, but none were very near the nucleus, where the column density of dust is highest. We report here unidentified emission bands, centered at λ4430, very near the nucleus of comet Hyakutake. These may be vaporized forms of grain carriers or fragments of large-molecule carriers. At least two different species appear to be present based on two different spatial distributions.

Keywords

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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