110 citations · 292 across the 4 of their papers we have counts for
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astro-ph.GA2017★ 54 cited
Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues II: Mg and Fe-rich amorphous silicates
K. Demyk, C. Meny, H. Leroux +5
To model the cold dust emission observed in the diffuse interstellar medium, in dense molecular clouds or in cold clumps that could eventually form new stars, it is mandatory to kn…
astro-ph.GA2017★ 72 cited
Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues I: Mg-rich glassy silicates
K. Demyk, C. Meny, X. -H. Lu +11
A wealth of data from the Herschel and Planck satellites and now from ALMA, revealing cold dust thermal emission, is available for astronomical environments ranging from interstell…
astro-ph.GA2011★ 110 cited
Low temperature FIR and submm mass absorption coefficient of interstellar silicate dust analogues
A. Coupeaud, K. Demyk, C. Meny +7
Cold dust grains emission in the FIR/submm is usually expressed as a modified black body law in which the dust mass absorption coefficient (MAC), is described with a temperature- a…