Rotational Properties of 21 SC Galaxies with a Large Range of Luminosities and Radii, from NGC 4605 (R = 4 kpc) to UGC 2885 (R = 122 kpc) (Scholarly article) (Q1557): Difference between revisions

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-W. Kent Ford
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@@ Property / attributed to: Vera Rubin / rank @@
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@@ Property / attributed to @@
+W. Kent Ford
@@ Property / attributed to: W. Kent Ford / rank @@
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@@ Property / attributed to @@
+Norbert Thonnard
@@ Property / attributed to: Norbert Thonnard / rank @@
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+Source:Rotational Properties of 21 SC Galaxies with a Large Range of Luminosities and Radii, from NGC 4605 (R = 4 kpc) to UGC 2885 (R = 122 kpc) (Scholarly article)

Latest revision as of 08:07, 3 September 2026

1980 paper by Vera Rubin, W. Kent Ford Jr. and Norbert Thonnard measuring optical rotation curves of 21 Sc spiral galaxies, showing they stay flat to the last measured point, far beyond where the visible light falls off — key evidence that spiral galaxies are embedded in dark matter halos

Language	Label	Description	Also known as
English	Rotational Properties of 21 SC Galaxies with a Large Range of Luminosities and Radii, from NGC 4605 (R = 4 kpc) to UGC 2885 (R = 122 kpc) (Scholarly article)	1980 paper by Vera Rubin, W. Kent Ford Jr. and Norbert Thonnard measuring optical rotation curves of 21 Sc spiral galaxies, showing they stay flat to the last measured point, far beyond where the visible light falls off — key evidence that spiral galaxies are embedded in dark matter halos