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Spectroscopic confirmation of two luminous galaxies at a redshift of 14 [PDF]
NatureAayush Saxena +2 more
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Compact E+A Galaxies as a Progenitor of Massive Compact Quiescent Galaxies at 0.2
2016Updated to accepted ...
Zahid, H. Jabran +7 more
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The nature of E and SO galaxies
Astrophysical letters & communications, 1995Differences and similarities of E and SO galaxies have been studied based on CCD surface photometry in Gunn r for a magnitude limited sample of E and SO galaxies in the Coma cluster. Spectroscopy is available for about half the sample. Our analysis of the relative disk luminosities, the Fundamental Plane, and the Mg-2-log sigma relation implies that E ...
Jorgensen, I, Franx, M
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Galaxy: A Gateway to Tools in e-Science
2011e-Science focuses on the use of computational tools and resources to analyze large scientific datasets. Performing these analyses often requires running a variety of computational tools specific to a given scientific domain. This places a significant burden on individual researchers for whom simply running these tools may be prohibitively difficult ...
Enis Afgan +5 more
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E and S0 Galaxies in the Perseus Supercluster
1989The Perseus Supercluster is a huge structure belonging to the Southern Galactic Hemisphere and probably extending to the Northern one [1]. It has been the subject of many different studies.
P. Focardi +3 more
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Dynamics of E Galaxies and Cluster Sources
1988Spherical stellar systems with large numbers of stars on nearly radial orbits are prone to be bar unstable. It seems likely that stars formed from a cooling flow tend to populate such orbits, thus ensuring that the underlying galaxy is barred; a simple estimate suggests that a mass deposition rate in excess of 5 M⊙ yr-1 should suffice for this purpose.
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A population of red candidate massive galaxies ~600 Myr after the Big Bang
Nature, 2023Rachel Bezanson +2 more
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Galaxies at redshifts 5 to 6 with systematically low dust content and high [C ii] emission
Nature, 2015Olivier Ilbert, Lin Yan, Karim A
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Molecular Clouds in Nearby Galaxies
Annual Review of Astronomy and Astrophysics, 2010Akiko Kawamura, Yasuo Fukui
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