Constraints on a Universal Stellar Initial Mass Function from Ultraviolet to Near‐Infrared Galaxy Luminosity Densities [PDF]
I. K. Baldry, Karl Glazebrook
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Reconciling M/L Ratios Across Cosmic Time: a Concordance IMF for Massive Galaxies
The stellar initial mass function (IMF) is thought to be bottom heavy in the cores of the most massive galaxies, with an excess of low-mass stars compared to the Milky Way.
Pieter van Dokkum, Charlie Conroy
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Galactic archaeology: initial mass function and depletion in the 'thin disc' [PDF]
Klaus‐Peter Schröder, B. E. J. Pagel
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We use large-scale cosmological simulations to study the prospect of observing Population III (Pop III) bright galaxies with the James Webb Space Telescope (JWST).
Richard Sarmento, Evan Scannapieco
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Hubble Space TelescopeNICMOS Observations of the Embedded Cluster in NGC 2024: Constraints on the Initial Mass Function and Binary Fraction [PDF]
Wilson Liu+3 more
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Missing Massive Stars in Starbursts: Stellar Temperature Diagnostics and the Initial Mass Function [PDF]
Jane R. Rigby, G. H. Rieke
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Mass to Light Ratio, Initial Mass Function, and Chemical Evolution in Disk Galaxies [PDF]
L. Portinari+2 more
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The Initial Mass Function and Stellar Content of NGC 3603 [PDF]
Hwankyung Sung, M. S. Bessell
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From Stars to Superplanets: The Low‐Mass Initial Mass Function in the Young Cluster IC 348
Joan Najita, G. P. Tiede, J. Carr
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Variability in the stellar initial mass function at low and high mass: three-component IMF models [PDF]
Bruce G. Elmegreen
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