What is the rate of star formation in the Milky Way?
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This strongly suggests that star formation in the Milky Way is a dynamic process on GMC scales. | |
Our results are consistent with observed galaxy stellar mass functions, specific star formation rates (SSFRs), and cosmic star formation rates (CSFRs) from z = 0 to z = 8. | |
The results for the star formation rate agree with recent observational data on early-type galaxies. | |
Our star formation rate (SFR) agrees well with those obtained by using other independent methods and seems to rule out a constant SFR. | |
the specific star formation rates in the host galaxies are generally consistent with those of normal star-forming (main sequence) galaxies; 2.) | |
We also show that the surface star formation rate profile of the Milky Way correlates well with the molecular gas surface density profile. | |
This has important implications for the determination of star formation rates in high-redshift galaxies. |
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