Results 151 to 160 of about 71,111 (245)
The Neutral Hydrogen Distribution in Spiral and Irregular Galaxies [PDF]
R. D. Davies
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"Fermi" bubbles are bursting from our galaxy. Their origins remain a mystery. [PDF]
Mann A.
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Are High-Σ1 Massive Blue Spiral Galaxies Rejuvenated Systems?
Quiescent galaxies generally possess denser cores than star-forming galaxies with similar mass. As a measurement of the core density, the central stellar mass surface density within a radius of 1 kpc (Σ _1 ) was thus suggested to be closely related to ...
Cai-Na Hao+7 more
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Gravitational potential of a disk spiral galaxy
B. Barbanis, K. H. Prendergast
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Impacts of Bar-driven Shear and Shocks on Star Formation
Bars drive gas inflow. As the gas flows inward, shocks and shear occur along the bar dust lanes. Such shocks and shear can affect the star formation (SF) and change the gas properties.
Taehyun Kim+14 more
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Numerical models of galaxies - I. The variability of spiral structure [PDF]
Robert H. Berman+2 more
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Surface photometry and mass distributions of spiral galaxies - I. NGC 157 [PDF]
C. P. Blackman
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Erratum: Southern Galaxies. V. Isophotometry of the Large Barred Spiral NGC 4945.
G. de Vaucouleurs
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