Results 61 to 70 of about 15,815 (162)

On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies

open access: yesThe Astrophysical Journal
Observed and simulated galaxies exhibit a significant variation in their velocity dispersion profiles. We examine the inner and outer slopes of stellar velocity dispersion profiles using integral field spectroscopy data from two surveys, SAMI (for z < 0 ...
San Han   +10 more
doaj   +1 more source

Strategies for Obtaining Robust Spectral Energy Distribution Fitting Parameters for Galaxies at z ∼ 1 and z ∼ 2 in the Absence of Infrared Data

open access: yesThe Astrophysical Journal
Robust estimation of star formation rates (SFRs) at higher redshifts ( z ≳ 1) using UV–optical–near-infrared (NIR) photometry is contingent on the ability of spectral energy distribution (SED) fitting to constrain the dust attenuation, stellar ...
Chandler Osborne, Samir Salim
doaj   +1 more source

Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at 0.7 ≲ z ≲ 9.3 with NIRSpec High-resolution Spectroscopy

open access: yesThe Astrophysical Journal Letters
The electron density ( n _e ) of the interstellar medium (ISM) in star-forming galaxies is intimately linked to star formation and ionization condition.
Sijia Li   +19 more
doaj   +1 more source

Induced galaxy formation

open access: yes, 2004
We describe the model of protogalaxy formation around the cluster of primordial black holes with a minimum extension of standard cosmological model. Namely, it is supposed, that a mass fraction of the universe ~10^-3 is composed of the compact clusters of primordial (relict) black holes produced during the phase transitions in the early universe. These
Dokuchaev, Vyacheslav   +2 more
openaire   +2 more sources

Formation of galaxies

open access: yesNuclear Physics B, 1985
Abstract The present theories of galaxy formation are reviewed. The relation between peculiar velocities and the correlation function of galaxies points to the possibility that galaxies do not form uniformly everywhere. Scale invariant properties of the cluster-cluster correlations are discussed. Comparing the correlation functions in a dimensionless
openaire   +1 more source

The Impact of Molecular Hydrogen Cooling on the Galaxy Formation Threshold

open access: yesThe Astrophysical Journal Letters
We study the impact of molecular (H _2 ) and atomic (H i ) hydrogen cooling on the galaxy formation threshold. We calculate the fraction of dark matter (DM) halos that exceeds a critical mass required for star formation, M _crit ( z ), as a function of ...
Ethan O. Nadler
doaj   +1 more source

Formation of Triaxial Galaxy [PDF]

open access: yesJournal of Astronomy and Space Sciences, 1987
Results of N-body simulation of dissipationless cold collapse of spherical gravitating system are presented. We compared the results with properties of elliptical galaxies. The system gradually evolved to triaxial system. The projected density profile is
Jang-Hyeon Park, Soo-Yong Kim
doaj  

Optical Spectroscopy of Dwarf Galaxies at z ∼ 0.15 in the COSMOS Field: Star Formation and Dust Properties

open access: yesThe Astrophysical Journal
We present a spectroscopic study of low-mass galaxies (LMGs;10 ^8 ≤ M _* / M _⊙ ≤ 10 ^9 ) at z  ∼ 0.15 in the Cosmic Evolution Survey field, and compare it to a control sample of intermediate-mass galaxies (IMGs; 10 ^9 ≤ M _* / M _⊙ ≤ 10 ^10 ) at z  ∼ 0 ...
Zahra Sattari   +6 more
doaj   +1 more source

Quasar Negative Feedback to Surrounding Galaxies Probed with Lyα Emitters and Continuum-selected Galaxies

open access: yesThe Astrophysical Journal Letters
We report on the statistical analysis of quasar photoevaporation at z  ∼ 2.2 by comparing the density of surrounding Ly α emitters (LAEs) and continuum-selected galaxies, based on the imaging data of the Hyper Suprime-Cam (HSC) Subaru Strategic Program ...
Yuta Suzuki   +5 more
doaj   +1 more source

Galaxy formation with BECDM - I. Turbulence and relaxation of idealized haloes. [PDF]

open access: yesMon Not R Astron Soc, 2017
Mocz P   +6 more
europepmc   +1 more source

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