Water Ice, Silicate, and Polycyclic Aromatic Hydrocarbon Emission Featuresin the [ITAL]Infrared Space Observatory[/ITAL] Spectrum of the Carbon-richPlanetary Nebula CPD −56°8032-Reference-Cited by-同舟云学术

Water Ice, Silicate, and Polycyclic Aromatic Hydrocarbon Emission Featuresin the [ITAL]Infrared Space Observatory[/ITAL] Spectrum of the Carbon-richPlanetary Nebula CPD −56°8032

Published:1999-03-10 Issue:2 Volume:513 Page:L135-L138
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
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Author:

Cohen Martin,Barlow M. J.,Sylvester R. J.,Liu X.-W.,Cox P.,Lim T.,Schmitt B.,Speck A. K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference40 articles.

1. 8-13 m spectra of very late type Wolf-Rayet stars

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

3. Barlow, M. J. 1993, in IAU Symp. 155, Planetary Nebulae, ed. R. Weinberger & A. Acker (Dordrecht: Kluwer), 163

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