We report new detailed surface U, B, V, R, and I photometry of 81 stellar structures in the disk of the barred galaxy NGC 3367. The images show many different structures, indicating that star formation is going on in most parts of the disk. NGC 3367 is known to have a very high concentration of molecular gas distribution in the central regions of the galaxy and bipolar synchrotron emission from the nucleus, with two lobes (at 6kpc) forming a triple structure similar to a radio galaxy. We have determined the U, B, V, R, and I magnitudes and U-B, B-V, U-V, and V-I colors for the central region (nucleus), a region which includes supernova 2003 AA, and 79 star associations throughout NGC 3367.

Cone search capability for table J/AJ/134/142/table3 (Our estimated UBVRI photometry of stars in M67 with IRAF phot, and those observed by other groups)

Cone search capability for table J/AJ/134/142/ngc3367 (UBVRI photometry of structures throughout NGC 3367, of stars and a background galaxy in the field of NGC 3367)