Abstract:
LSB galaxies are metal poor, have diffuse stellar disks and massive HI disks. We have detected molecular gas in two giant LSB galaxies, UGC 6614 and F568-6. A millimeter continuum source has been detected in UGC 6614 as well. At centimeter wavelengths we have detected and mapped the continuum emission from the giant LSB galaxy 1300+0144. The emission is extended about the nucleus and is most likely originating from the AGN in the galaxy. The HI gas distribution and velocity eld in 1300+0144 was also mapped. The HI disk extends well beyond the optical disk and appears to be lopsided in the intensity maps.

Paper - astro-ph/0609426