The spatial distribution of emission from the unidentified infrared bands View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1995

AUTHORS

F. O. Clark , Rob Assendorp , Paul Wesselius , Peter Roelfsema , Kester , R. F. Shipman , Thomas A. Kuchar , M. P. Egan , R. L. Phelps

ABSTRACT

The IRAS focal plane contained a slitless spectrometer, the Low Resolution Spectrometer (LRS). Several regions in the Rosette nebula HII region are nearly unresolved in the in-scan direction, permitting extraction of LRS spectra. The spectral coverage of the LRS includes some of the unidentified infrared (UIR) bands, associated with PAHs by some authors. The extracted spectra include three clearly defined regimes: low density ionized material, of order 30 cm−3, non-ionized material of the same density, and denser material with equivalent luminosity of an embedded early B star. Only the last exhibit UIR emission bands in our data. More... »

PAGES

156-157

Book

TITLE

The Physics and Chemistry of Interstellar Molecular Clouds

ISBN

978-3-540-60482-2

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bfb0102123

DOI

http://dx.doi.org/10.1007/bfb0102123

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1011828254


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