Dust in Low Surface Brightness Galaxies

Details Dust in Low Surface Brightness Galaxies Dust in Low Surface Brightness Galaxies

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...62r&link_type=abstract

Spitzer Proposal ID #62

Computer Science

Scientific paper

Low surface brightness galaxies may represent a significant component of the baryonic matter in the Universe. However, these galaxies appearto have followed a very different star formation history fromhigh surface brightness galaxies. IRAS was able to detect a coupleof these galaxies as was ISO, but enough data to characterizethe dust temperature and spatial distribution were not acquired.This project uses MIPS photometry mode to detect the dust ina sample of LSB galaxies chosen to have low cirrus and sufficientlylarge angular diameters for resolution by MIPS.

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