The PAH Hypothesis after 25 Years - Wikidata - wikimedia - TriplyDB

The PAH Hypothesis after 25 Years

The PAH Hypothesis after 25 Years

http://www.wikidata.org/entity/Q57673835

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Ion-induced molecular growth in clusters of small hydrocarbon chains

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P2860

The PAH Hypothesis after 25 Years

http://www.wikidata.org/entity/Q57673835

description

wetenschappelijk artikel

@nl

наукова стаття, опублікована в червні 2011

@uk

name

The PAH Hypothesis after 25 Years

@en

The PAH Hypothesis after 25 Years

@nl

type

label

The PAH Hypothesis after 25 Years

@en

The PAH Hypothesis after 25 Years

@nl

prefLabel

The PAH Hypothesis after 25 Years

@en

The PAH Hypothesis after 25 Years

@nl

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S174392131102494X

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Proceedings of the International Astronomical Union

P1476

The PAH Hypothesis after 25 Years

@en

P2093

Els Peeters

http://www.w3.org/2001/XMLSchema#string

P2860

Variations in the Peak Position of the 6.2 μm Interstellar Emission Feature: A Tracer of N in the Interstellar Polycyclic Aromatic Hydrocarbon Population

SINGS: The SIRTF Nearby Galaxies Survey

Photodissociation of [Fe(x)(C24H12)y]+ complexes in the PIRENEA setup: iron-polycyclic aromatic hydrocarbon clusters as candidates for very small interstellar grains.

Detection of C60 and C70 in a young planetary nebula.

Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications.

TheSpitzer/GLIMPSE Surveys: A New View of the Milky Way

The NASA ames polycyclic aromatic hydrocarbon infrared spectroscopic database: the computed spectra

The 15–20 μm PAH emission features: probes of individual PAHs?

Unusual dust emission from planetary nebulae in the Magellanic clouds

The infrared spectra of very large irregular polycyclic aromatic hydrocarbons (PAHs): observational probes of astronomical PAH geometry, size, and charge

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149-161

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scholarly article

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10.1017/S174392131102494X

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S280

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7

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2011-06-01T00:00:00Z

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1111.3680

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