Cold dust in M31 as mapped by ISO

Details Cold dust in M31 as mapped by ISO Cold dust in M31 as mapped by ISO

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000immm.proc...69h&link_type=abstract

The interstellar medium in M31 and M33. Proceedings 232. WE-Heraeus Seminar, 22-25 May 2000, Bad Honnef, Germany. Edited by El

Computer Science

Scientific paper

This contribution addresses the following topics: (1) The ISO 175 micron
map: a ring-like dust distribution (2) Two dust components with the
dominance of much cold dust (3) What causes M31's ring structure and how
will it evolve? (4) Search for dust in the outer disk beyond 14 kpc
radius. First results have been reported in Haas et al. (1998).

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