1k citations · 1.9k across the 19 of their papers we have counts for
19 papers
On the importance of scattering at 8 microns: Brighter than you think
Charlène Lefèvre, Laurent Pagani, Michiel Min +2
Context. Extinction and emission of dust models need for observational constraints to be validated. The coreshine phenomenon has already shown the importance of scattering in the 3…
The Composition of Interstellar Grains Toward Zeta Ophiuchi: Constraining the Elemental Budget Near the Diffuse-Dense Cloud Transition
Charles A. Poteet, Douglas C. B. Whittet, Bruce T. Draine
We investigate the composition of interstellar grains along the line of sight toward Zeta Ophiuchi, a well-studied environment near the diffuse-dense cloud transition. A spectral d…
Observations of the Icy Universe
Adwin Boogert, Perry Gerakines, Douglas Whittet
Freeze-out of the gas phase elements onto cold grains in dense interstellar and circumstellar media builds up ice mantles consisting of molecules that are mostly formed in situ (H2…
Extended High Circular Polarization in the Orion Massive Star Forming Region: Implications for the Origin of Homochirality in the Solar System
Tsubasa Fukue, Motohide Tamura, Ryo Kandori +7
We present a wide-field (~6'x6') and deep near-infrared (Ks band: 2.14 micro m) circular polarization image in the Orion nebula, where massive stars and many low-mass stars are for…
Understanding Polarized Foreground from Dust: Towards Reliable Measurements of CMB Polarization
Alex Lazarian, Dan Clemens, Andy Adamson +16
Science opportunities and recommendations concerning optical/infrared polarimetry for the upcoming decade in the field of cosmology. Community-based White Paper to Astro2010 in res…
Near-Infrared Circular Polarimetry and Correlation Diagrams in the Orion BN/KL Region: Contribution of Dichroic Extinction
T. Fukue, M. Tamura, R. Kandori +8
We present a deep circular polarization image of the Orion BN/KL nebula in the Ks band and correlations of circular polarization, linear polarization, and H-Ks color representing e…