Results 21 to 30 of about 235,164 (217)
The accretion of galaxies into groups and clusters [PDF]
We use the galaxy stellar mass and halo merger tree information from the semi-analytic model galaxy catalogue of Font et al. (2009) to examine the accretion of galaxies into a large sample of groups and clusters, covering a wide range in halo mass (10E12.9 to 10E15.3 Msun/h), and selected from each of four redshift epochs (z=0, 0.5, 1.0 and 1.5).
McGee, SL +4 more
openaire +3 more sources
Dust accretion and destruction in galaxy groups and clusters [PDF]
Dust accretion and destruction in galaxy groups and ...
Sean L. Mcgee +3 more
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Galaxy Dynamics: Secular Evolution and Accretion [PDF]
Recent results are reviewed on galaxy dynamics, bar evolution, destruction and re-formation, cold gas accretion, gas radial flows and AGN fueling, minor mergers. Some problems of galaxy evolution are discussed in particular, exchange of angular momentum,
Francoise Combes, Combes, Françoise
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Modelling and observations of molecules in discs around young stars [PDF]
This thesis contains a study of molecules within circumstellar discs around young stars. Firstly, the chemistry of a disc around a young, Class 0 protostar is modelled.
Ilee, John David
core +5 more sources
Galaxy growth through accretion and mergers [PDF]
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutor: Alberto Manrique OlivaGalaxies have been the main protagonist in Cosmology and the study of the Universe for almost a century. Currently, they have become
Villegas Pelegrín, Sergio-Yersi
core +4 more sources
MaNGA 8313-1901 : gas accretion observed in a blue compact dwarf galaxy [PDF]
Gas accretion is an important process in the evolution of galaxies, but it has limited direct observational evidences. In this paper, we report the detection of a possible ongoing gas accretion event in a blue compact dwarf (BCD) galaxy, MaNGA 8313-1901,
Telles, Jose Eduardo +15 more
core +1 more source
Abstract In the two-phase scenario of galaxy formation, a galaxy’s stellar mass growth is first dominated by in-situ star formation, and subsequently by accretion. We analyze the radial distribution of the accreted stellar mass in ∼500 galaxies from the (48 Mpc/h)3 box volume of the hydrodynamical cosmological simulation Magneticum, in a
Rhea-Silvia Remus, Duncan A. Forbes
openaire +3 more sources
Evidence for Recent Accretion in Nearby Galaxies [PDF]
I discuss observations of magnitude residuals from the B-band Tully-Fisher relationship, B-V color, chemical abundance gradients, and asymmetries in the H I and stellar disks of nearby spiral galaxies within the context of a model in which small satellites or H I clouds are accreted onto the outer disks of spiral galaxies.
openaire +2 more sources
Galaxy masses play a fundamental role in our understanding of structure formation models. This review addresses the variety and reliability of mass estimators that pertain to stars, gas, and dark matter.
Courteau, Stephane +10 more
core +1 more source
Galaxy And Mass Assembly (GAMA) : galaxy close pairs, mergers and the future fate of stellar mass [PDF]
ASGR acknowledges STFC and SUPA funding that were used to do this work. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO and the participating institutions.We use a highly complete subset of the Galaxy And Mass Assembly II (GAMA-II) redshift
De Propris, R. +130 more
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