The recent star formation (SF) in the early-type spiral galaxy M81 is characterized using imaging observations from the far-ultraviolet to the far-infrared. We compare these data with models of the stellar, gas, and dust emission for subgalactic regions.
Cone search capability for table J/ApJ/648/987/table1 (Positions and photometry (GLOBALBKG and LOCALBKG cases) for the regions selected at 160um resolution)
Cone search capability for table J/ApJ/648/987/table2 (Positions and photometry for the regions selected at 24um resolution)