The Tully-Fisher relation for low surface brightness galaxies: implications for galaxy evolution
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The Core-Cusp ProblemModified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic ExtensionsUniversality of galactic surface densities within one dark halo scale-length.Radial Acceleration Relation in Rotationally Supported Galaxies.From distances to galaxy evolution and the dark matter problemThe MASSIVE survey – III. Molecular gas and a broken Tully–Fisher relation in the most massive early-type galaxiesCombined Solar system and rotation curve constraints on MOND
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The Tully-Fisher relation for low surface brightness galaxies: implications for galaxy evolution
description
im März 1995 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в березні 1995
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name
The Tully-Fisher relation for ...... lications for galaxy evolution
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The Tully-Fisher relation for ...... lications for galaxy evolution
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type
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The Tully-Fisher relation for ...... lications for galaxy evolution
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The Tully-Fisher relation for ...... lications for galaxy evolution
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The Tully-Fisher relation for ...... lications for galaxy evolution
@en
The Tully-Fisher relation for ...... lications for galaxy evolution
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P2093
P356
P1476
The Tully-Fisher relation for ...... lications for galaxy evolution
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J. M. van der Hulst
M. A. Zwaan
W. J. G. de Blok
P304
P356
10.1093/MNRAS/273.1.L35
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P577
1995-03-01T00:00:00Z
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P818
astro-ph/9501102