Abundance ratios in dwarf elliptical galaxies [PDF]
We determine abundance ratios of 37 dwarf ellipticals (dEs) in the nearby Virgo cluster. This sample is representative of the early-type population of galaxies in the absolute magnitude range -19.0 < Mr < -16.0. We analyze their absorption line-strength indices by means of index-index diagrams and scaling relations and use the stellar population ...
Jesús Falcón-Barroso+21 more
openaire +10 more sources
Structural properties of discs and bulges of early-type galaxies [PDF]
We have used the EFAR sample of galaxies to study the light distributions of early-type galaxies. We decompose the 2D light distribution of the galaxies in a flattened spheroidal component with a Sersic radial light profile and an inclined disc component
Abell+85 more
core +4 more sources
Equilibrium Figures inside the Dark-Matter Ring and the Shapes of Elliptical Galaxies
We solve the general problem of the theory of equilibrium figures and analyze two classes of liquid rotating gravitating figures residing inside a gravitating ring or torus.
Kondratyev B. P.+2 more
doaj +1 more source
Resolving the Extended Stellar Halos of Nearby Galaxies: The Wide-Field PISCeS Survey
The wide-field Panoramic Imaging Survey of Centaurus and Sculptor (PISCeS) investigates the resolved stellar halos of two nearby galaxies (the spiral NGC 253 and the elliptical Centaurus A, D ∼ 4 Mpc) out to a galactocentric radius of 150 kpc ...
Denija Crnojević
doaj +1 more source
A binary model for the UV-upturn of elliptical galaxies (MNRAS version) [PDF]
The discovery of a flux excess in the far-ultraviolet (UV) spectrum of elliptical galaxies was a major surprise in 1969. While it is now clear that this UV excess is caused by an old population of hot helium-burning stars without large hydrogen-rich ...
A. E. Lynas-Gray+162 more
core +4 more sources
Properties of Early-Type, Dry Galaxy Mergers and the Origin of Massive Elliptical Galaxies [PDF]
The luminosity dependence of kinematical and isophotal properties of elliptical galaxies is investigated using numerical simulations of galaxy merging, combined with semi-analytical models of hierarchical structure formation. Mergers of spiral galaxies as the only formation mechanism for elliptical galaxies can neither reproduce the kinematical and ...
arxiv +1 more source
The baryonic haloes of elliptical galaxies: radial distribution of globular clusters and diffuse hot gas [PDF]
For a sample of nine well-studied giant ellipticals, we compare the projected radial distribution of their red and blue globular cluster (GC) subpopulations with their host galaxy stellar and X-ray surface brightness profiles.
D. Forbes, T. Ponman, E. O’Sullivan
semanticscholar +1 more source
The Distribution Of Heavy Elements In Spiral And Elliptical Galaxies [PDF]
This review recaps significant results as they apply to non-dwarf galaxies, including the Milky Way, spiral disks and bulges, and elliptical and lenticular galaxies. Conclusions that span the galaxy types treated here are as follows.
Arimoto N.+53 more
core +2 more sources
Binary Stellar Population Synthesis Study of Elliptical Galaxies [PDF]
We determine relative stellar ages and metallicities mainly for about 80 elliptical galaxies in low and high density environments via the latest binary stellar population (BSP) synthesis model and test a latest hierarchical formation model of elliptical galaxies which adopted the new $\Lambda$CDM cosmology for the first time.
arxiv +1 more source
On the distribution of galaxy ellipticity in clusters [PDF]
14 pages, 11 figures, Accepted for publication in ...
Rebecca Davies+4 more
openaire +5 more sources