Results 61 to 70 of about 32,916 (218)
The Complex Structure of the Bulge of M31
The bulge of M31 is of interest regarding the nature of galactic bulges and how their structure relates to bulge formation mechanisms and their subsequent evolution.
Denis Leahy +2 more
doaj +1 more source
Structures in Galaxy Clusters [PDF]
(16 pages in LATEX, 4 tables in LATEX are at the end of the file, the figures not included are available upon request), REF SISSA 158/93 ...
Escalera, E. +6 more
openaire +3 more sources
The clustering of dark matter, haloes & galaxies [PDF]
In this thesis I study the spatial distribution of galaxies, haloes and dark matter particles using a suite of state-of-art cosmological N-body simulations of the growth structure in the Universe.
Angulo de la Fuente, Raúl Esteban
core
A large-scale galaxy structure at z = 2.02 associated with the radio galaxy MRC 0156-252 [PDF]
We present the spectroscopic confirmation of a structure of galaxies surrounding the radio galaxy MRC 0156-252 at z = 2.02. The structure was initially discovered as an overdensity of both near-infrared selected z > 1.6 and mid-infrared selected z > 1.2 ...
Rettura, A. +36 more
core +1 more source
The edge of the Milky Way’s star-forming disc: Evidence from a ’U-shaped’ stellar age profile
We leveraged reliable age and distance estimates from LAMOST-DR3 and APOGEE-DR17+AstroNN combined with Gaia data to perform a detailed analysis of the stellar age distribution in the Milky Way’s (MW) outer disc using giant stars. Selecting stars near the
Fiteni Karl +9 more
doaj +1 more source
THE ROLE OF POOR GALAXY CLUSTERS FOR STUDYING SUPERCLUSTER STRUCTURE
The distribution of galaxy clusters is analyzed in regions of 6 galaxy superclusters with both measured and estimated redshifts. The positions of ACO and APM galaxy clusters in the regions are compared with the positions of galaxy clusters and groups ...
E. A. Panko
doaj +1 more source
Simulating molecular cloud regulated star formation in Galaxies [PDF]
This thesis is primarily concerned with understanding the process of galaxy formation via the simulation of the interstellar medium, star formation and supernova feedback.
Booth, Craig Martin
core
Early assembly of the most massive galaxies [PDF]
The current consensus is that galaxies begin as small density fluctuations in the early Universe and grow by in situ star formation and hierarchical merging(1).
Chris A. Collins +53 more
core +1 more source
Line-of-Sight Structure Toward Strong Lensing Galaxy Clusters
Spectroscopic and photometric catalogs of galaxies analyzed in Bayliss et al. study of line of sight structure toward strong lensing galaxy clusters. There are two types of ASCII tables, one containing the photometric and redshift data for each galaxy ...
Matthew B Bayliss
core +1 more source
MHD numerical simulations in a cosmological context [PDF]
Magnetic fields in the Universe are found in almost all studied environments. In particular, their presence in the inter-galactic medium and in the intra-cluster medium is confirmed by diffuse radio emission as well as by observations of Faraday ...
Stasyszyn, Federico Andrés +1 more
core

