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Modes of the Dark Ages 21 cm field accessible to a lunar radio interferometer. [PDF]
Bull P, Guandalin C, Addis C.
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Revisiting the Surface Brightness Profile of the Stellar Disk with the Statistical Mechanics of the Self-Gravitating System with the Central Body. [PDF]
Kang DB.
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Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P+21 more
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Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D+21 more
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Controlling the motion of gravitational spinners and waves in chiral waveguides. [PDF]
Kandiah A+3 more
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Spin-orbit-splitting-driven nonlinear Hall effect in NbIrTe4. [PDF]
Lee JE+15 more
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Dynamics of Elliptical Galaxies
Science, 1993Elliptical galaxies were once thought to be similar in their structure and dynamics to rotationally flattened bodies like stars. The discovery that elliptical galaxies rotate much more slowly than a fluid body with the same shape has led to a qualitative change in our understanding of the dynamics of these systems.
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Anatomy of elliptical galaxies
Nature, 2009The family of elliptical galaxies is remarkable for the structural regularity of its members. Inspecting irregularities in this regularity could help in understanding how these galaxies form.
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