Cold dust in M33

Details Cold dust in M33 Cold dust in M33

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.482...79h&link_type=abstract

ISOPHOT: Proceedings of the Workshoip on P32 Oversampled Mapping, held in Madrid, Spain and Pasadena, CA, USA in February and Ma

Computer Science

1

Iso, Macros: Dust, Star Formation

Scientific paper

The Sc galaxy M 33 was mapped with ISO at three far in- frared wavelengths, 60, 100, and 160 μm, in order to study the distribution and the heating of dust. On the basis of a prelimi- nary data reduction done prior to the availability of P32TOOLS the spectral energy distributions in the FIR indicate the pres- ence of two dust components. The warmer component, at 40K,is concentrated to the star-forming regions, and heated by UV radiation from massive stars, thus tracing the star forma- tion activity, while the cold component, at 17K,is smoothly distributed over the entire disk, and which is heated by the dif- fuse interstellar radiation field.

Affiliated with

Also associated with

No associations

Rating

Cold dust in M33 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cold dust in M33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cold dust in M33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-963362