Results 21 to 30 of about 3,405,157 (289)
Constraining the Initial Mass Function via Stellar Transients
The stellar initial mass function (IMF) represents a fundamental quantity in astrophysics and cosmology describing the mass distribution of stars from low mass all the way up to massive and very massive stars. It is intimately linked to a wide variety of
Francesco Gabrielli +6 more
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The relationship between the prestellar core mass function and the stellar initial mass function [PDF]
7 pages, 3 figures, A&A in ...
Goodwin, S. P. +4 more
openaire +7 more sources
We use recent microlensing observations toward the central bulge of the Galaxy to probe the overall stellar plus brown dwarf initial mass function (IMF) in these regions well within the brown dwarf domain. We find that the IMF is consistent with the same
Gilles Chabrier, Romain Lenoble
doaj +1 more source
The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster
The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local validity of general
Ilaria Lonoce +2 more
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Variation of the High-mass Slope of the Stellar Initial Mass Function: Theory Meets Observations
We present observational evidence of a correlation between the high-mass slope of the stellar initial mass function (IMF) in young star clusters and their stellar surface density, σ _* .
Sami Dib
doaj +1 more source
Mapping the core mass function to the initial mass function [PDF]
13 pages, 15 figures, accepted by MNRAS on 17 April ...
Guszejnov, Dávid, Hopkins, Philip F.
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Low-mass stars and substellar objects are essential in tracing the initial mass function (IMF). We study the nearby young σ Orionis cluster ( d ∼ 408 pc, age ∼ 1.8 Myr) using deep near-infrared (NIR) photometric data in the J , W , and H bands from ...
Belinda Damian +13 more
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THE HIGH-MASS STELLAR INITIAL MASS FUNCTION IN M31 CLUSTERS [PDF]
11 pages, 7 Figures, submitted to ApJ.
Daniel R. Weisz +18 more
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This work presents and releases a catalog of new photometrically derived physical properties for the ∼10 ^5 most well-measured galaxies in the COSMOS field on the sky.
Vadim Rusakov +2 more
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Fragmentation and the initial mass function [PDF]
A central problem in the theory of star formation is to understand the spectrum of masses, or Initial Mass Function, with which stars are formed. The fundamental role of the IMF in galactic evolution has been described by Tinsley (1980), and an extensive review of evidence concerning the IMF and its possible variability has been presented by Scalo ...
openaire +1 more source

