STAR FORMATION IN THE OUTER RESONANCE RING OF NGC 1300

摘要

Surface photometry of the barred galaxy NGC 1300 in B and I bands reveals an outer pseudo-ring with star formation knots located at the positions of 10~8 solar mass H I clouds previously mapped by M. England with the VLA. The age of the ring from the B-I colors is estimated to be ～10~9 yr, and the age of the star formation knots is estimated to be ～2 x 10~7 yr. Stability considerations suggest that the H I clouds formed by gravitational condensation along the ring periphery. If the outer extent of the ring is at the outer Lindblad resonance, then the bar ends slightly outside the inner 4:1 resonance and coro-tation is at the position of the break and dust lane crossing midway out in the spiral arms.