Results 231 to 240 of about 12,786 (266)

Computational Cosmology: from the Early Universe to the Large Scale Structure. [PDF]

Living Rev Relativ, 1998
Anninos P.
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Quasi-Normal Modes of Stars and Black Holes. [PDF]

Living Rev Relativ, 1999
Kokkotas KD, Schmidt BG.
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Rotating stars in relativity. [PDF]

Living Rev Relativ, 2017
Paschalidis V, Stergioulas N.
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Magellanic Clouds: IV. On the Period Frequency Anomalies. [PDF]

Proc Natl Acad Sci U S A, 1952
Shapley H, Nail VM.
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Galactic and Extragalactic Studies: II. Notes on the Peculiar Stellar Systems in Sculptor and Fornax. [PDF]

Proc Natl Acad Sci U S A, 1939
Shapley H.
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Magellanic Clouds: VI. Revised Distances and Luminosities. [PDF]

Proc Natl Acad Sci U S A, 1953
Shapley H.
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The dynamics of dwarf spheroidal galaxies

, 2018
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Inhomogeneous chemical evolution of dwarf spheroidal galaxies

Astrophysics and Space Science, 2003
Stellar abundance pattern of n-capture elements such as barium is used as a powerful tool to infer how the star formation proceeded in dwarf spheroidal (dSph) galaxies. It is found that the abundance correlation of barium with iron in stars belonging to dSph galaxies orbiting the Milky Way, i.e., Draco, Sextans, and Ursa Minor have a feature similar to
Takuji Tsujimoto, Toshikazu Shigeyama
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Dwarf Spheroidal Galaxies: Dynamical Evolution

Astrophysics and Space Science, 1998
We show the results of numerical simulations of dwarf spheroidal galaxies (DSphs), which allow to understand their evolution in the framework of no internal virial equilibrium. Under this hypothesis, we reproduce with a low dark matter (DM) model the high values of the virial M/L ratio measured observationally for these objects.
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Searches for dwarf spheroidal galaxies

Astrophysics, 1975
1. Dwarf spheroidal galaxies are encountered, it would seem, more often than previously assumed [9]. 2. The tendency for them to be concentrated around galaxies of high luminosities [8, 9] is not very pronounced. 3. The distribution of Sculptor type dwarfs in the space we studied is not uniform.
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