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Spectropolarimetry of the 3.4 μm Feature in the Diffuse ISM toward the Galactic Center Quintuplet Cluster

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J. E. Chiar1, A. J. Adamson2, D. C. B. Whittet3, A. Chrysostomou4, J. H. Hough4, T. H. Kerr2, R. E. Mason5, P. F. Roche6 and G. Wright7

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[1]

H Atom Irradiation of Carbon Grains under Simulated Dense Interstellar Medium Conditions: The Evolution of Organics from Diffuse Interstellar Clouds to the Solar System

Vito Mennella  The Astrophysical Journal 2010  718 867
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[2]

Oxygen Depletion in the Interstellar Medium: Implications for Grain Models and the Distribution of Elemental Oxygen

D. C. B. Whittet  The Astrophysical Journal 2010  710 1009
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[3]

Polarized Far-Infrared and Submillimeter Emission from Interstellar Dust

Bruce T. Draine and Aurélien A. Fraisse  The Astrophysical Journal 2009  696 1
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[4]

Obscuration in Extremely Luminous Quasars

M. Polletta et al.  The Astrophysical Journal 2008  675 960
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[5]

Electronic and Vibrational Spectroscopy of Diamondoids and the Interstellar Infrared Bands between 3.35 and 3.55 μm

Charles W. Bauschlicher, Jr. et al.  The Astrophysical Journal 2007  671 458
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[6]

Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era

B. T. Draine and Aigen Li  The Astrophysical Journal 2007  657 810
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[7]

Spectropolarimetry of the 3.4 μm Absorption Feature in NGC 1068

R. E. Mason et al.  The Astrophysical Journal 2007  656 798
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