Axially Symmetric Superwinds of Proto–Planetary Nebulae with 21 Micron Dust Features

Arens, J F; Skinner, C. J.; Meixner, M.; Graham, J. R.; Jernigan, J. G.; Keto, E.

doi:10.1086/304174

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Axially Symmetric Superwinds of Proto–Planetary Nebulae with 21 Micron Dust Features

Author(s): M. Meixner , C. J. Skinner , J. R. Graham , E. Keto , J. G. Jernigan , J. F. Arens

Publication date Created: June 20 1997

Publication date (Print): June 20 1997

Journal: The Astrophysical Journal

Publisher: University of Chicago Press

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

G. Tielens, L. J. Allamandola, J R Barker (1989)

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etal; (1997)

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Shape and clustering effects on the optical properties of amorphous carbon

Francois Rouleau, P. G. Martin (1991)

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Journal

Title: The Astrophysical Journal

Abbreviated Title: ApJ

Publisher: University of Chicago Press

ISSN (Print): 0004-637X

ISSN (Electronic): 1538-4357

Publication date Created: June 20 1997

Publication date (Print): June 20 1997

Volume: 482

Issue: 2

Pages: 897-912

Article

DOI: 10.1086/304174

SO-VID: b8fd3060-f46b-4993-807d-6ebfba8d17af

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Axially Symmetric Superwinds of Proto–Planetary Nebulae with 21 Micron Dust Features

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Most cited references 37

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

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Shape and clustering effects on the optical properties of amorphous carbon

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