Comment on “The shape and composition of interstellar silicate grains”
Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, Livermore, CA 94550, USA e-mail: email@example.com
Accepted: 4 April 2008
This article has no abstract.
Key words: astrochemistry / solar system: general / ISM: dust, extinction
© ESO, 2008