(Q59096819)

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Laboratory evidence for highly unsaturated hydrocarbons as carriers ofsome of the diffuse interstellar bands

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Laboratory evidence for highly unsaturated hydrocarbons as carriers ofsome of the diffuse interstellar bands (English)

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J. Fulara

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1

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D. Lessen

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P. Freivogel

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3

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J. P. Maier

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English

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publication date

December 1993

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Nature

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volume

366

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issue

6454

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page(s)

439-441

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https://scigraph.springernature.com/pub.10.1038/366439a0

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The diffuse interstellar bands. IV - The region 4400-6850 A

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Diffuse interstellar bands — an observational review (Review)

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New diffuse interstellar bands in the wavelength region 6500-8900 A

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The diffuse interstellar bands. VI. New features near 6800 A

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Detection of diffuse interstellar bands in the infrared

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The diffuse interstellar bands. VIII. New features between 6000 and 8650 A

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Origin of diffuse interstellar lines

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The ultraviolet and visible spectrum of the polycyclic aromatic hydrocarbon C10H8+ : possible contributions to the diffuse interstellar bands and to the ultraviolet-visible extinction

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Is a pyrene-like molecular ion the cause of the 4,430-angstroms diffuse interstellar absorption band?

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Is interstellar detection of higher members of the linear radicals CnCH and CnN feasible?

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Chemical abundances in cold, dark interstellar clouds

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The detection of butadiynyl (C4 H) in absorption against Cassiopeia A

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10.1038/366439A0

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1005046830

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(Q59096819)

Laboratory evidence for highly unsaturated hydrocarbons as carriers ofsome of the diffuse interstellar bands

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