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Interplay of dust alignment, grain growth, and magnetic fields in polarization: lessons from the emission-to-extinction ratio

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Evolution of dust extinction curves in galaxy simulation

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Polyaromatic disordered carbon grains as carriers of the UV bump: Far-UV to mid-IR spectroscopy of laboratory analogs

L. Gavilan, K. C. Le, T. Pino, et al.
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Structure and infrared spectra of hydrocarbon interstellar dust analogs

Germán Molpeceres, Vicente Timón, Miguel Jiménez-Redondo, et al.
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Conel M. O'D. Alexander, Larry R. Nittler, Jemma Davidson and Fred J. Ciesla
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High Radiation Pressure on Interstellar Dust Computed by Light-scattering Simulation on Fluffy Agglomerates of Magnesium-silicate Grains with Metallic-iron Inclusions

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The Astrophysical Journal Letters 839 (2) L23 (2017)
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ASSESSMENT OF MODELS OF GALACTIC THERMAL DUST EMISSION USING COBE/FIRAS AND COBE/DIRBE OBSERVATIONS

N. Odegard, A. Kogut, D. T. Chuss and N. J. Miller
The Astrophysical Journal 828 (1) 16 (2016)
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Using cm observations to constrain the abundance of very small dust grains in Galactic cold cores

C. T. Tibbs, R. Paladini, K. Cleary, et al.
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The evolution of hydrocarbon dust grains in the interstellar medium and its influence on the infrared spectra of dust

M. S. Murga, S. A. Khoperskov and D. S. Wiebe
Astronomy Reports 60 (7) 669 (2016)
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Polarizing efficiency as a guide of grain growth and interstellar magnetic field properties

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Absorption at 11 μm in the interstellar medium and embedded sources: evidence for crystalline silicates

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