File:Parenago-discontinuity.png

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Revision as of 22:33, 5 May 2019 by Johnno (talk | contribs) (Velocity dispersion of 12,000 main-sequence stars versus colour. The abrupt change in slope at (B−V) = 0.6 is called Parenago’s discontinuity. From Binney, Dehnen & Bertelli (2000).)
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Velocity dispersion of 12,000 main-sequence stars versus colour. The abrupt change in slope at (B−V) = 0.6 is called Parenago’s discontinuity. From Binney, Dehnen & Bertelli (2000).

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current22:33, 5 May 2019Thumbnail for version as of 22:33, 5 May 2019660 × 568 (16 KB)Johnno (talk | contribs)Velocity dispersion of 12,000 main-sequence stars versus colour. The abrupt change in slope at (B−V) = 0.6 is called Parenago’s discontinuity. From Binney, Dehnen & Bertelli (2000).

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