Galaxy rotation curve/Bibliography: Difference between revisions
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Pat Palmer (talk | contribs) (Created page with "{{subpages}} * {{cite journal | author=V. Rubin, W. K. Ford, Jr| title= Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions | journal=Astrophysical Journal | year=1970 | volume=159 | pages=379}} *: This was the first detailed study of orbital rotation in galaxies. * {{cite journal | author=V. Rubin, W. K. Ford, Jr, N. Thonnard | title= Rotational Properties of 21 Sc Galaxies with a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc...") |
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Latest revision as of 10:39, 28 June 2024
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- V. Rubin, W. K. Ford, Jr (1970). "Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions". Astrophysical Journal 159: 379.
- This was the first detailed study of orbital rotation in galaxies.
- V. Rubin, W. K. Ford, Jr, N. Thonnard (1980). "Rotational Properties of 21 Sc Galaxies with a Large Range of Luminosities and Radii from NGC 4605 (R=4kpc) to UGC 2885 (R=122kpc)". Astrophysical Journal 238: 471.
- Observations of a set of spiral galaxies gave convincing evidence that orbital velocities of stars in galaxies were unexpectedly high at large distances from the nucleus. This paper was influential in convincing astronomers that most of the matter in the universe is dark, and much of it is clumped about galaxies.
- Galactic Dynamics, James Binney and Scott Tremaine.Princeton University Press 1987. ISBN 0-691-08444-0 (cloth); ISBN 0-691-08445-9 (paperback)
- J. R. Brownstein and J. W. Moffat (2006). "Galaxy Rotation Curves Without Non-Baryonic Dark Matter". Astrophysical Journal 636: 721.
- Arxiv.org Preprint (astro-ph/0506370)