Implications of a Temperature Dependent IMF I: Photometric Template Fitting
Autor: | Sneppen, Albert, Steinhardt, Charles L., Hensley, Hagan, Jermyn, Adam S., Mostafa, Basel, Weaver, John R. |
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Rok vydání: | 2022 |
Předmět: | |
Druh dokumentu: | Working Paper |
DOI: | 10.3847/1538-4357/ac695e |
Popis: | A universal stellar initial mass function (IMF) should not be expected from theoretical models of star formation, but little conclusive observational evidence for a variable IMF has been uncovered. In this paper, a parameterization of the IMF is introduced into photometric template fitting of the COSMOS2015 catalog. The resulting best-fit templates suggest systematic variations in the IMF, with most galaxies exhibiting top-heavier stellar populations than in the Milky Way. At fixed redshift, only a small range of IMFs are found, with the typical IMF becoming progressively top-heavier with increasing redshift. Additionally, subpopulations of ULIRGs, quiescent- and star-forming galaxies are compared with predictions of stellar population feedback and show clear qualitative similarities to the evolution of dust temperatures. Comment: Published in the 'The Astrophysical Journal' |
Databáze: | arXiv |
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