Results 151 to 160 of about 517,834 (312)
The Outer Halos of Elliptical Galaxies [PDF]
Recent progress is summarized on the determination of the density distributions of stars and dark matter, stellar kinematics, and stellar population properties, in the extended, low surface brightness halo regions of elliptical galaxies. With integral field absorption spectroscopy and with planetary nebulae as tracers, velocity dispersion and rotation ...
openaire +2 more sources
Ionized gas in the nuclei of elliptical, so, spiral, and irregular galaxies [PDF]
Ionized gas in elliptical, SO, spiral, and irregular galaxy ...
Burbidge, E. M., Burbidge, G. R.
core +1 more source
The Elliptical Galaxy formerly known as the Local Group: Merging the Globular Cluster Systems [PDF]
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
core +3 more sources
Stellar Populations of Elliptical Galaxies in Virgo Cluster. I. The Data and Stellar Population Analysis [PDF]
Y. Yamada +3 more
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Nuclear stellar discs in low-luminosity elliptical galaxies: NGC 4458 and 4478 [PDF]
L. Morelli +9 more
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The Elliptical-Spheroidal and Elliptical-Elliptical Galaxy Dichotomies
8 pages, 4 figures, requires asp2006.sty, to be published in Galaxy Evolution: Emerging Insights and Future Challenges, ed. S. Jogee et al., Astron. Soc.
openaire +2 more sources
On the Formation of Elliptical Galaxies [PDF]
Simple collapse and violent relaxation models produce sharply cut off envelopes with ϱ(r) ∝ r–4, whereas actual elliptical galaxies have more extended envelopes approximately given by ϱ(r) ∝ r–3 as implied by Hubble's Law. Numerical models are presented, showing that when cosmological infall effects are included, galaxies are produced with more ...
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Motion of Stars in Layered Inhomogeneous Elliptical Galaxies [PDF]
S. А. Gasanov
openalex +1 more source
VV 191 is a nearby ( z ∼ 0.05), overlapping (occulting) galaxy pair, where a multiple-armed spiral galaxy is backlit by an elliptical galaxy. The overlap is used to derive and map dust attenuation in two James Webb Space Telescope NIRCam filters (F090W ...
Clayton D. Robertson +10 more
doaj +1 more source
Absorption Line Gradients of an Elliptical Galaxy NGC 5322 [PDF]
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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