Results 51 to 60 of about 4,025,746 (356)

The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations [PDF]

open access: yes, 2018
We propose a novel method to constrain the missing fraction of galaxies using galaxy clustering measurements in the galaxy conditional stellar mass function (CSMF) framework, which is applicable to surveys that suffer significantly from sample selection ...
Hong Guo, Xiaohu Yang, Yi Lu
semanticscholar   +1 more source

Dynamics of Dwarf Galaxies Disfavor Stellar-Mass Black Holes as Dark Matter. [PDF]

open access: yesPhysical Review Letters, 2017
We study the effects of black hole dark matter on the dynamical evolution of stars in dwarf galaxies. We find that mass segregation leads to a depletion of stars in the center of dwarf galaxies and the appearance of a ring in the projected stellar ...
S. Koushiappas, A. Loeb
semanticscholar   +1 more source

Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies

open access: yes, 2018
Using deep images from the Hyper Suprime-Cam (HSC) survey and taking advantage of its unprecedented weak lensing capabilities, we reveal a remarkably tight connection between the stellar mass distribution of massive central galaxies and their host dark ...
Ardila, Felipe   +11 more
core   +1 more source

The stellar mass-halo mass relation of isolated field dwarfs : a critical test of ΛCDM at the edge of galaxy formation [PDF]

open access: yes, 2016
We fit the rotation curves of isolated dwarf galaxies to directly measure the stellar mass-halo mass relation (M*-M200) over the mass range 5 × 105 ≲ M*/M⊙ ≲ 108.
J. Read   +5 more
semanticscholar   +1 more source

ON THE MAXIMUM MASS OF STELLAR BLACK HOLES [PDF]

open access: yesThe Astrophysical Journal, 2010
15 pages, ApJ ...
Jarrod R. Hurley   +9 more
openaire   +5 more sources

Extragalactic Constraints on the Initial Mass Function [PDF]

open access: yes, 2008
The local stellar mass density is observed to be significantly lower than the value obtained from integrating the cosmic star formation history (SFH), assuming that all the stars formed with a Salpeter initial mass function (IMF).
Adelman-McCarthy   +24 more
core   +4 more sources

Effect of Local Environment and Stellar Mass on Galaxy Quenching and Morphology at 0.5 < z < 2.0 [PDF]

open access: yes, 2017
We study galactic star formation activity as a function of environment and stellar mass over 0.5 < z < 2.0 using the FourStar Galaxy Evolution (ZFOURGE) survey.
L. Kawinwanichakij   +22 more
semanticscholar   +1 more source

The evolution of the stellar mass versus halo mass relationship [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We present an analysis of the predictions made by the Galform semi-analytic galaxy formation model for the evolution of the relationship between stellar mass and halo mass. We show that for the standard implementations of supernova feedback and gas reincorporation used in semi-analytic models, this relationship is predicted to evolve weakly over the ...
Mitchell, Peter D.   +3 more
openaire   +5 more sources

What Is the Role of Stellar Radiative Feedback in Setting the Stellar Mass Spectrum? [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract In spite of decades of theoretical efforts, the physical origin of the stellar initial mass function (IMF) is still debated. Particularly crucial is the question of what sets the peak of the distribution. To investigate this issue, we perform high-resolution numerical simulations with radiative feedback exploring, in particular,
Benoît Commerçon   +4 more
openaire   +5 more sources

Red Galaxy Growth and the Halo Occupation Distribution

open access: yes, 2008
We have traced the past 7 Gyr of red galaxy stellar mass growth within dark matter halos. We have determined the halo occupation distribution, which describes how galaxies reside within dark matter halos, using the observed luminosity function and ...
Andrew J. Benson   +15 more
core   +1 more source

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