Duty Cycle and the Exponentially Increasing History of Star Formation of z>=6 Galaxies

Mathematics – Logic

Scientific paper

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Scientific paper

Using cosmological hydrodynamic simulations, we find good consistency between the simulations and observed photometric properties of z=9 to z=6 galaxies, such as the color-color diagrams and rest-frame UV luminosity function. By performing a fit to the Schechter luminosity function we find an evolving faint-end luminosity slope of -2.00 and steeper for z=6 to z=9, suggesting a significant population of small faint galaxies which are currently beyond our observational limits. Motivated by our concurrence with the observed photometric properties, we explore the duty cycle, star formation histories (SFH) and number densities of these high-z galaxies. We find that although individual galaxies have bursty SFH, the mean SFH show a clear exponentially increasing SFH with time-scales ranging from 70 Myr to 200 Myr for galaxies with Mstar=106 to 1010 Msun. We also calculate the duty cycle of star formation above an observable star formation threshold, and find that it makes a steep transition from zero to unity between Mstar=107 to 109 Msun.

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