Absorption Line Gradients of an Elliptical Galaxy NGC 5322 [PDF]
Journal of Astronomy and Space Sciences, 1999 Archival long-slit spectra, covering the wavelength range 4050Å - 5150Å, have been used to investigate the radial behavior of absorption line features (G4300, Fe4383, Ca4455, Fe44531, Fe4668, and Hα) of an eliptical galaxy NGC 5322.
Young-Jong Sohn +2 more
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Stellar Population Synthesis of the Elliptical Galaxy NGC 4649 [PDF]
Journal of Astronomy and Space Sciences, 2001 We investigated population of the elliptical galaxy NGC 4649 using the spectral synthesis technique based on the linear program in the spectral regions between 3160Å to 10800Å. We used the spectral data of stars obtained by Gunn & Stryker (1983), and the
Mun-Suk Chun +2 more
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Deep imaging with Milanković telescope: Linking merger history to kinematics of elliptical galaxies [PDF]
, 2023 Ivana Ebrová +6 more
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The Elliptical Galaxy formerly known as the Local Group: Merging the Globular Cluster Systems [PDF]
, 2000 Prompted by a new catalogue of M31 globular clusters, we have collected together individual metallicity values for globular clusters in the Local Group. Although we briefly describe the globular cluster systems of the individual Local Group galaxies, the
Barmby, Pauline +3 more
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A New Dynamical Parameter for the Study of Sticky Orbits in a 3D Galactic Model
Open Astronomy, 2011 A 3D dynamical model is used to study the motion in the central parts of an elliptical galaxy, hosting a massive and dense nucleus. Our aim is to investigate the regular or chaotic character of the motion, with emphasis in the different chaotic ...
Zotos Euaggelos E.
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Direct IR Determination of the Stellar Luminosity Function to 0.2 M⊙ in Elliptical Galaxies [PDF]
, 1987 G. Gilmore, K. A. Arnaud
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Galaxy evolution: the effect of dark matter on the chemical evolution of ellipticals and galaxy clusters [PDF]
, 1996 F. Matteuccí, B. K. Gibson
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Evolution of Massive Red Galaxies in Clusters from z = 1.0 to z = 0.3
The Astronomical JournalA critical issue in studying the evolution of galaxy clusters is to find ways that enable meaningful comparisons of clusters observed at different redshifts, as well as in various stages of their growth.
Yen-Ting Lin +4 more
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Dissipationless mergers of elliptical galaxies and the evolution of the fundamental plane [PDF]
, 2005 Michael Boylan-Kolchin +2 more
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No Evidence of a Dichotomy in the Elliptical Galaxy Population
The Astrophysical JournalThe advent of large integral field spectroscopic surveys has found that elliptical galaxies (EGs) can be divided into two classes: the fast rotators (whose kinematics are dominated by rotation) and the slow rotators (which exhibit slow or no rotation ...
Rogério Monteiro-Oliveira +5 more
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