Infrared Cooling in an Anharmonic Cascade Framework: 2-Cyanoindene, the Smallest Cyano-PAH Identified in Taurus Molecular Cloud-1. [PDF]
Stockett MH+4 more
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Battle of the CH motions: aliphatic versus aromatic contributions to astronomical PAH emission and exploration of the aliphatic, aromatic, and ethynyl CH stretches. [PDF]
Esposito VJ+5 more
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Constraining the history of water and climate on Mars through light element stable isotope analysis of volatiles in returned martian samples. [PDF]
Grady MM.
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Diversity of protonated mixed pyrene-water clusters investigated by collision induced dissociation.
M Nair A+7 more
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The Onset of Axial Symmetry in Protoplanetary Nebulae
Astrophysics and Space Science, 1995We have obtained resolved IR images, at wavelengths from 1.2μm to 12.5μm, of a small sample of protoplanetary nebulae. The results suggest that all PPNe are axially, not spherically, symmetric, that spherical symmetry ends at the tip of the AGB, and that AGB evolution terminates with a burst of remarkably rapid, equatorially concentrated mass-loss.
M. J. Barlow+5 more
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The Dust Subdisk in the Protoplanetary Nebula
Icarus, 1995Abstract We present a self-consistent computation of the structure of the dust subdisk in the protoplanetary nebula. The main physical processes governing the dynamics of the dust disk are reviewed. A (nonlinear) vertical diffusion equation for the transport of dust particles is derived.
Gregor E. Morfill+2 more
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Compact reflection nebulae associated with protoplanetary nebulae
Chinese Astronomy and Astrophysics, 1991Abstract Optical identifications and slit spectra and CCD direct images show that, of the protoplanetary nebulae (PPN) selected from the IRAS Catalogue of Point Sources, three are associated with compact reflection nebulae. In this paper we use a spherically symmetric dust shell model to calculate the brightness and colour evolution of the central ...
Hu Jing-yao, Tang Qing-quan
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Formation of amorphous ice in the protoplanetary nebula
Planetary and Space Science, 1994Abstract The criteria for formation of amorphous ice in different models of the protoplanetary nebula are developed. Assuming that comets are composed mostly of amorphous ice, it is shown that the inner boundary of formation of cometary nuclei is about 7 A.U.
Y. Mekler, Morris Podolak
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