Spiral Molecular Front in Galaxies: Quick Transition from Atomic to Molecular Hydrogen in Spiral Arms

We derived a two-dimensional map of the molecular fraction, fmol, (ratio of the molecular gas density to that of total gas) in the spiral galaxy M51, and examined the behavior of molecular fronts (MF), where MF represents the place where fmol changes drastically from nearly zero to unity and vice versa. We show that the MF phenomenon occurs not only radial, but also in the azimuth direction through the spiral arms, and fmol changes rapidly in the arm-to-inter-arm transition regions. The existence of the azimuthal MF indicates that the atomic gas (HI) is quickly transformed to molecular gas (H2) during the passage through spiral arms. We performed a numerical simulation of MF based on an HI-to-H2 phase transition theory, and reproduced the observations. We estimated a azimuthal scale length of the transition to be less than 200 pc, corresponding to a time scale of ∼ 2 Myr for H2 gas formation. The azimuthal width of a molecular arm is estimated to be at most 2.5 kpc, where the gas can remain in molecular phase for about 25 Myr. Kew words: galaxies: spiral — galaxies: ISM — galaxies: cluster of — Molecular gas — HI gas