Chemical Evolution of the Galaxy Based on the Oscillatory Star Formation History

Abstract

We model the star formation history (SFH) and the chemical evolution of the Galactic disk by combining an infall model and a limit-cycle model of the interstellar medium (ISM). Recent observations have shown that the SFH of the Galactic disk violently variates or oscillates. We model the oscillatory SFH based on the limit-cycle behavior of the fractional masses of three components of the ISM. The observed period of the oscillation ($\sim 1$ Gyr) is reproduced within the natural parameter range. This means that we can interpret the oscillatory SFH as the limit-cycle behavior of the ISM. We then test the chemical evolution of stars and gas in the framework of the limit-cycle model, since the oscillatory behavior of the SFH may cause an oscillatory evolution of the metallicity. We find however that the oscillatory behavior of metallicity is not prominent because the metallicity reflects the past integrated SFH. This indicates that the metallicity cannot be used to distinguish an oscillatory SFH from one without oscillations.

arXiv comment21 pages LaTeX, to appear in ApJ

References in corpus (12)

• The Global Schmidt Law in Star Forming Galaxies
• The Chemical Evolution of the Galaxy: the two-infall model
• Low-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution
• The metallicity distribution of G dwarfs in the solar neighbourhood
• The recent star formation history of the Hipparcos solar neighbourhood
• An Intermittent Star Formation History in a 'Normal' Disk Galaxy: The Milky Way
• The mass surface density in the local disk and the chemical evolution of the Galaxy
• A Variation of the Present Star Formation Activity of Spiral Galaxies
• Intermittent Star-Formation Activities of Dwarf Irregular Galaxies
• Application of the Limit Cycle Model to Star Formation Histories in Spiral Galaxies: Variation among Morphological Types
• Testing Intermittency of the Galactic Star Formation History along with the Infall Model
• Metal Enrichment in the Early Galactic Halo

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