INSPIRE: INvestigating Stellar Population In RElics IV. The Initial Mass Function slope in relics
I. Martin-Navarro, C. Spiniello, C. Tortora, L. Coccato, G. D'Ago, A., Ferre-Mateu, C. Pulsoni, J. Hartke, M. Arnaboldi, L. Hunt, N. R. Napolitano,, D. Scognamiglio, M. Spavone

TL;DR
This study compares the stellar initial mass function in relic galaxies versus non-relics, providing evidence that relics have a systematically bottom-heavier IMF, supporting the idea of IMF non-universality and its link to early star formation conditions.
Contribution
It presents the first detailed spectral analysis of relic galaxies, showing they have a bottom-heavier IMF than similar non-relic galaxies, supporting theories of IMF variation.
Findings
Relics exhibit a systematically bottom-heavier IMF slope.
Non-relics show a more extended star formation history.
Supports the non-universality of the IMF across different galaxy types.
Abstract
In the last decade, growing evidence has emerged supporting a non-universal stellar Initial Mass Function (IMF) in massive galaxies, with a larger number of dwarf stars with respect to the Milky-Way (bottom-heavy IMF). However, a consensus about the mechanisms that cause IMF variations is yet to be reached. Recently, it has been suggested that stars formed early-on in cosmic time, via a star formation burst, could be characterised by a bottom-heavy IMF. A promising way to confirm this is to use relics, ultra-compact massive galaxies, almost entirely composed by these "pristine" stars. The INSPIRE Project aims at assembling a large sample of confirmed relics, that can serve as laboratory to investigate on the conditions of star formation in the first 1-3 Gyr of the Universe. In this third INSPIRE paper, we build a high signal-to-noise spectrum from five relics and one from five galaxies…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
