Robert Hugh Sanders
Affiliations: | 1970 | Princeton University, Princeton, NJ | |
| 1989-2010 | Astronomy | University of Groningen, Groningen, Netherlands |
Area:
active galactic nucleiWebsite:
http://www.rug.nl/staff/r.h.sanders/Google:
"Robert Hugh Sanders"Bio:
http://hoogleraren.ub.rug.nl/hoogleraren/2164-sanders-robert-h-bob
http://adsabs.harvard.edu/abs/1970PhDT.........6S
http://articles.adsabs.harvard.edu//full/1970ApJ...162..791S/0000809.000.html
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Parents
Sign in to add mentor| Lyman Spitzer | grad student | 1970 | Princeton | |
| (On the Coalescence of Colliding Stars in Dense Stellar Systems.) | ||||
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Publications
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| Milgrom M, Sanders RH. (2003) MOND and the 'Dearth of dark matter in ordinary elliptical galaxies' The Astrophysical Journal. 599 |
| Bekenstein JD, Milgrom M, Sanders RH. (2000) Comment on "The bright side of dark matter" Physical Review Letters. 85: 1346 |
| Breimer TG, Sanders RH. (1992) Constraints on cosmological parameters from clusters containing luminous arcs Monthly Notices of the Royal Astronomical Society. 257: 97-104 |
| Lemson G, Sanders R. (1991) On the use of the conditional density as a description of galaxy clustering Monthly Notices of the Royal Astronomical Society. 252: 319-328 |
| Begeman K, Broeils A, Sanders R. (1991) Extended rotation curves of spiral galaxies: dark haloes and modified dynamics Monthly Notices of the Royal Astronomical Society. 249: 523-537 |
| Sanders RH. (1990) Mass discrepancies in galaxies: dark matter and alternatives The Astronomy and Astrophysics Review. 2: 1-28 |
| Sanders R. (1989) Cosmological implications of phase coupling gravity Monthly Notices of the Royal Astronomical Society. 241: 135-151 |
| Sanders RH. (1989) Noncircular Gas Motions In The Inner Galaxy Iau Symposia. 77-87 |
| Sanders R. (1988) Phase coupling gravity and astronomical mass discrepancies Monthly Notices of the Royal Astronomical Society. 235: 105-121 |
| Soares D, Sanders R. (1987) The Distribution And Kinematics Of Stars Formed From The Cooling Flow In M87 Monthly Notices of the Royal Astronomical Society. 229: 119-128 |