Results 121 to 130 of about 3,870 (231)
BL Lac Host Galaxies: How to Systematically Characterize Them in Optical–Near-infrared Spectroscopy
Host galaxies of active galactic nuclei (AGN) give crucial information on the interaction between accreting supermassive black holes and their surroundings and on their common evolution.
Gaia Delucchi +5 more
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Gradients of absorption line indices are studied and mean stellar metallicities are estimated for 46 elliptical galaxies. The mean stellar metallicities range from [[Fe/H]] similar or equal to -0.8 to +0.2 and ellipticals with smaller central velocity ...
Arimoto, N, Kobayashi, Chiaki
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Cold Gas and Star Formation in Elliptical Galaxies
. Elliptical galaxies outside dense clusters are observed to contain small amounts (relative to spiral galaxies) of cold interstellar gas. This review discusses the atomic gas, the molecular gas, and the dust in elliptical galaxies.
Gillian Knapp
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WHY EXTENDED RADIO DOUBLES ARE FOUND IN ELLIPTICAL GALAXIES
[[abstract]]Elliptical galaxies rotate very slowly, and this rotation affects the way in which gas lost from stars finds its way into the nucleus. It is suggested that the dynamical nature of this flow is the reason why extended double radio sources ...
SPARKE, L.S.;SHU, F.H.
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Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGA
Using “spatially” resolved spectroscopy, we investigated the characteristics and different modes of formation of stars in elliptical galaxies. We identified an unusual population of 59 star-forming elliptical (SF-E) galaxies in SDSS-MaNGA, our primary ...
Pralay Biswas, Yogesh Wadadekar
doaj +1 more source
An Improved Distance Indicator for Elliptical Galaxies
We present a new relation between velocity dispersion, surface brightness, and radius (or luminosity) for elliptical galaxies. Relative distances of galaxies can be estimated to within 0.13 in log D.
Djorgovski, S., Davis, Marc
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Understanding the CNO cycle and the proton-proton (p-p) chain is essential for comprehending the development of main sequence stars in the initial stages of spiral and elliptical galaxy formation. This study investigates two nuclear reactions that occur
Rabab Muzhir J., Al Najm M. N.
doaj +1 more source
The centers of massive elliptical galaxies exhibit a wide range in density profiles, from central cusps to resolved cores with order kiloparsec sizes.
Kyle Kremer +4 more
doaj +1 more source
The origin of elliptical galaxies inferred from their metallicity gradients
We simulate the chemodynamical evolution of elliptical galaxies using our GRAPE-SPH code. We succeed in reproducing the observed variety of the radial metallicity gradients, from which we discuss the origin of elliptical ...
Kobayashi, C
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In this thesis, a sample of nearby, compact, elliptical galaxies with high central stellar velocity dispersions are studied. By means of high quality photometric and spectroscopic observations, we analyse their structural properties and construct state ...
Yildirim, Akin
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