Cold dust in M33

Details Cold dust in M33 Cold dust in M33

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000immm.proc...81h&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

1

Scientific paper

The Sc galaxy M33 was mapped with ISO at three far infrared wavelengths, 60, 100, and 170 micron, in order to study the distribution and the heating of dust. The spectral energy distribution in the FIR indicates to be composed of two components. A warmer component at ~ 40 K, more concentrated to the star-forming regions, and a cold component at ~ 17 K, which is smoothly distributed all over the disk, but also seen in the dense star forming regions, and which is heated by the diffuse interstellar radiation.

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