Was the Milky Way a chain galaxy? Using the IGIMF theory to constrain the thin-disk star formation history and mass
Akram Hasani Zonoozi, Hamidreza Mahani, Pavel Kroupa

TL;DR
This study uses the IGIMF theory to analyze the star formation history and mass of the Milky Way's thin disk, suggesting it may have appeared as a chain galaxy in the early universe.
Contribution
It constrains the Milky Way's star formation rate, history, and mass using the IGIMF framework, linking stellar populations to galaxy evolution.
Findings
Current SFR estimated at 4.1 M_sun/yr
Declining star formation history inferred
Galactic mass and stellar remnants quantified
Abstract
The observed present-day stellar mass function (PDMF) of the solar neighborhood is a mixture of stellar populations born in star-forming events that occurred over the life-time of the thin disk of the Galaxy. Assuming stars form in embedded clusters which have stellar initial mass functions (IMFs) which depend on the metallicity and density of the star-forming gas clumps, the integrated galaxy-wide IMF (IGIMF) can be calculated. The shape of the IGIMF thus depends on the SFR and metallicity. Here, the shape of the PDMF for stars more massive than in combination with the mass density in low-mass stars is used to constrain the current star-formation rate (SFR), the star formation history (SFH) and the current stellar plus remnant mass () in the Galactic thin disk. This yields the current SFR, yr, a declining SFH and…
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