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Formation, Evolution and Properties of Isolated Field Elliptical Galaxies [PDF]

open access: yes, 2010
[Abridged] We study the properties, evolution and formation mechanisms of isolated field elliptical galaxies. We create a mock catalogue of isolated field elliptical galaxies from the Millennium Simulation Galaxy Catalogue, and trace their merging ...
Aars   +59 more
core   +4 more sources

Confirmation of Enhanced Dwarf-sensitive Absorption Features in the Spectra of Massive Elliptical Galaxies: Further Evidence for a Non-universal Initial Mass Function [PDF]

open access: yes, 2011
We recently found that massive cluster elliptical galaxies have strong Na I 8183,8195 and FeH 9916 Wing-Ford band absorption, indicating the presence of a very large population of stars with masses
Buitrago   +18 more
core   +2 more sources

A new method for the identification of non-Gaussian line profiles in elliptical galaxies

open access: green, 1993
A new parameterization for the line profiles of elliptical galaxies, the Gauss-Hermite series, is proposed. This approach expands the line profile as a sum of orthogonal functions which minimizes the correlations between the errors in the parameters of ...
Roeland P. van der Marel, Marijn Franx
openalex   +2 more sources

The Relationship between Slope and Luminosity [PDF]

open access: yesKirkuk Journal of Science, 2010
In this study, a sample of galaxies has been adopted. It consists of 112 elliptical galaxies, among them were 56 dwarf elliptical galaxies, which belong to virgo cluster, 37 normal galaxies and 19 bright galaxies. Also, surface brightness profiles fitted
Mohsen H. Ali AL-Khafajy
doaj   +1 more source

Deviations of the Surface Brightness Distribution in Isolated Elliptical Galaxies [PDF]

open access: yesمجلة التربية والعلم, 2012
In this paper, we present the surface brightness profiles of 48 isolated elliptical galaxies. we have adopted the r1/n – law to the observed surface brightness profiles of the adopted sample of isolated elliptical galaxies for the intermediate radial ...
Omar Salih
doaj   +1 more source

Planetary Nebulae and the Ionization of the Interstellar Medium in Galaxies

open access: yesFrontiers in Astronomy and Space Sciences, 2022
We discuss the role of planetary nebulae and their progeny in galaxy context in terms of ionization of the galaxy interstellar medium. This regards ionized gas outside the disk of spiral galaxies, the diffuse ionized medium in spiral galaxies, and the ...
Grażyna Stasińska   +2 more
doaj   +1 more source

Isolated compact elliptical galaxies: Stellar systems that ran away [PDF]

open access: yesScience, 2015
Galaxies stripped down and evicted It is easy to imagine that the relatively small and dense compact elliptical galaxies once had more to them. Especially when massive galactic neighbors are seen nearby that may have robbed them of their matter, but ...
I. Chilingarian, I. Zolotukhin
semanticscholar   +1 more source

The Fate of the Interstellar Medium in Early-type Galaxies. II. Observational Evidence for Morphological Quenching

open access: yesThe Astrophysical Journal, 2023
The mechanism by which galaxies stop forming stars and get rid of their interstellar medium (ISM) remains elusive. Here, we study a sample of more than 2000 elliptical galaxies in which dust emission has been detected.
Aleksandra Leśniewska   +6 more
doaj   +1 more source

The structural and dynamical properties of compact elliptical galaxies [PDF]

open access: yes, 2017
Dedicated photometric and spectroscopic surveys have provided unambiguous evidence for a strong stellar mass-size evolution of galaxies within the last 10 Gyr.
A. Yıldırım   +7 more
semanticscholar   +1 more source

Why there are no elliptical galaxies more flattened than E7: Thirty years later [PDF]

open access: yesSerbian Astronomical Journal, 2006
Elliptical galaxies are modeled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) where the peculiar velocity distribution is anisotropic, or equivalently as their adjoint configurations i.e.
Caimmi R.
doaj   +1 more source

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