FAR-INFRARED PROPERTIES OF LOCAL STAR-FORMING GALAXIES FROM THE UCM SAMPLE

The Universidad Complutense de Madrid Survey (UCM Survey) has been carried out the last years with the aim of lookingfor H α emission-line galaxies. ISO observed some of the UCM galaxies with different instruments but a very high percentage of these star-forming galaxies were observed in ISOPHOT Serendipity Mode. The objective is to get 175µm flux densities for as many objects as possible of the UCM Sample to collect more information about the FIR properties and the star formation processes through the comparison with all the optical data already available.