Results 41 to 50 of about 574,458 (198)

The significant effects of stellar mass estimation on galaxy pair fractions [PDF]

open access: yes, 2020
There exist discrepancies in measurements of the number and evolution of galaxy pairs. The pair fraction appears to be sensitive to both the criteria used to select pair fraction and the methods used to analyze survey data. This paper explores the connection between stellar mass estimation and the pair fraction of galaxies making use of STEEL, the ...
arxiv   +1 more source

Clustering properties of galaxies selected in stellar mass: Breaking down the link between luminous and dark matter in massive galaxies from z=0 to z=2 [PDF]

open access: yes, 2010
We present a study on the clustering of a stellar mass selected sample of 18,482 galaxies with stellar masses M*>10^10M(sun) at redshifts 0 ...
Arnaud   +139 more
core   +1 more source

Dark against Luminous Matter around Isolated Central Galaxies: A Comparative Study between Modern Surveys and IllustrisTNG

open access: yesThe Astrophysical Journal, 2023
Based on independent shear measurements using the Dark Energy Camera Legacy Survey/DR8 imaging data, we measure the weak lensing signals around isolated central galaxies (ICGs) from Sloan Digital Sky Survey/DR7 at z ∼ 0.1.
Pedro Alonso   +8 more
doaj   +1 more source

Reconciling observed and simulated stellar halo masses [PDF]

open access: yes, 2018
We use cosmological hydrodynamical simulations of Milky-Way-mass galaxies from the FIRE project to evaluate various strategies for estimating the mass of a galaxy's stellar halo from deep, integrated-light images.
Chan, Tsang Keung   +8 more
core   +5 more sources

Mass Measurements of Stellar and Intermediate-Mass Black Holes [PDF]

open access: yesSpace Science Reviews, 2013
28 pages, 12 figures. Accepted for publication in Space Science Reviews (DOI 10.1007/s11214-013-0030-6). Also to appear in hard cover in the Space Sciences Series of ISSI "The Physics of Accretion onto Black Holes" (Springer Publisher).
Jorge Casares   +4 more
openaire   +8 more sources

The Eclipsing Binaries from the LAMOST Medium-resolution Survey. III. A High-precision Empirical Stellar Mass Library

open access: yesThe Astronomical Journal, 2023
High-precision stellar masses and radii measured directly from binaries can effectively calibrate stellar models. However, such a database containing full spectral types and a large range of metallicity is still not fully established. A continuous effort
Jianping Xiong   +8 more
doaj   +1 more source

Stellar pulsations excited by a scattered mass [PDF]

open access: yesPhysical Review D, 1999
23 pages, 6 figures ...
FERRARI, Valeria   +2 more
openaire   +5 more sources

Tracing the Evolution of SMBHs and Stellar Objects in Galaxy Mergers: A Multi-mass Direct N-body Model

open access: yesThe Astrophysical Journal, 2023
By using direct N -body numerical simulations, we model the dynamical coevolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to investigate how different stellar components evolve during the merger, we
Shuo Li   +5 more
doaj   +1 more source

Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts [PDF]

open access: yes, 2019
We investigate the locations of satellite galaxies in the z = 0 redshift slice of the hydrodynamical Illustris-1 simulation. As expected from previous work, the satellites are distributed anisotropically in the plane of the sky, with a preference for ...
Brainerd, Tereasa G., Yamamoto, Masaya
core   +1 more source

Star formation and the origin of stellar masses [PDF]

open access: yesNature, 1992
AbstractWe present a new model to explain stellar mass distributions in different stellar environments. In our model, the protostar phase is terminated, when the protostellar core embedded in a molecular clump experiences a collision with another star or protostellar clump, which ejects the protostellar core from its parent clump.
Podsiadlowski, P, Price, N
openaire   +4 more sources

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