The Star Formation Rate in disk galaxies: thresholds and dependence on gas amount

Details The Star Formation Rate in disk galaxies: thresholds and dependence on gas amount The Star Formation Rate in disk galaxies: thresholds and dependence on gas amount

2003-09-13

arxiv.org/abs/astro-ph/0309372v1

Mon.Not.Roy.Astron.Soc.346:1215,2003

Astronomy and Astrophysics

Astrophysics

18 pages, 12 figures, accepted in MNRAS

Scientific paper

10.1111/j.1365-2966.2003.07170.x

We reassess the applicability of the Toomre criterion in galactic disks and we study the local star formation law in 16 disk galaxies for which abundance gradients are published. The data we use consists of stellar light profiles, atomic and molecular gas (deduced from CO with a metallicity-dependent conversion factor), star formation rates (from H-alpha emissivities), metallicities, dispersion velocities and rotation curves. We show that the Toomre criterion applies successfully to the case of the Milky Way disk, but it has limited success with the data of our sample; depending on whether the stellar component is included or not in the stability analysis, we find average values for the threshold ratio of the gas surface density to the critical surface density in the range 0.5 to 0.7. We also test various star formation laws proposed in the literature, i.e. either the simple Schmidt law or modifications of it, that take into account dynamical factors. We find only small differences among them as far as the overall fit to our data is concerned; in particular, we find that all three SF laws (with parameters derived from the fits to our data) match particularly well observations in the Milky Way disk. In all cases we find that the exponent n of our best fit SFR has slightly higher values than in other recent works and we suggest several reasons that may cause that discrepancy.

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