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Oxford University Press

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A Model for the Changing Pore Structure and Dust Grain Size Distribution in a Porous Comet Nucleus

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Interstellar extinction and polarization – a spheroidal dust grain approach perspective

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Dust growth in the interstellar medium: how do accretion and coagulation interplay?

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Monthly Notices of the Royal Astronomical Society, Vol. 422, Iss. 2, 2012-05 ,pp. : 1263-1271

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On the dust abundance gradients in late-type galaxies – II. Analytical models as evidence for massive interstellar dust growth in SINGS galaxies

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