Dust Properties in the Local Interstellar Medium

Details Dust Properties in the Local Interstellar Medium Dust Properties in the Local Interstellar Medium

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ssrv...97..389m&link_type=abstract

Space Science Reviews, v. 97, Issue 1/4, p. 389-392 (2001).

Computer Science

2

Scientific paper

Ulysses measurements yield reliable in-situdetection of large dust particles which stem from the interstellar medium (ISM) and which are not observed in interstellar extinction data. Both current models of large grains in the ISM: core-mantle grains as well as composite grains, are in agreement with dust properties implied by the Ulysses results. However, the size of particles detected by Ulysses still exceeds the size of the large grains that are predicted for the ISM.

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