
- MODIFIED NEWTONIAN DYNAMICS AS AN ALTERNATIVE TO DARK MATTER
- Seeing Through Dark Matter Stacy McGaugh
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- Balance of Dark and Luminous Mass in Rotating Galaxies Stacy S. McGaugh
- Cleveland Museum of Natural History, 9 December 2010 The Driving Role of Gravity in Cosmology
- MOND N-body: why a = p a 0 g N isn't enough
- The Mass Discrepancy Problem: New Physics in Matter or Gravity?
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- Accepted to ApJ Preprint typeset using LATEX style emulateapj v. 03/07/07
- HIGH-RESOLUTION OPTICAL VELOCITY FIELDS OF 11 LOW SURFACE BRIGHTNESS GALAXIES Rachel Kuzio de Naray1
- THE COMPRESSION OF DARK MATTER HALOS BY BARYONIC INFALL J. A. Sellwood
- THE BARYONIC TULLY-FISHER RELATION OF GALAXIES WITH EXTENDED ROTATION CURVES AND THE STELLAR MASS OF ROTATING GALAXIES
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- Modified Gravity Approaches to the Dark Sector 28 June 2010 Empirical Tests of MOND in Galaxies
- Dark Galaxies & Missing Baryons Proceedings IAU Symposium No. 244, 2007
- Advances in Theoretical and Observational Cosmology Maryland Center for Fundamental Physics & Joint Space-Science Institute 26-28 May 2010
- Cosmic Flights of Fancy: Mass and the Gravity that Moves It
- The Pros and Cons of Invisible Mass and Modified Gravity
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- Observational Constraints on the Acceleration Discrepancy Problem
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- SIR --It has recently been noted1 that a large variety of observations constrain cosmo-
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- CO DETECTION AND MILLIMETER CONTINUUM EMISSION FROM LOW SURFACE BRIGHTNESS GALAXIES
- DOES LOW SURFACE BRIGHTNESS MEAN LOW DENSITY? W. J. G. DE BLOK
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- THE MASS DISCREPANCYACCELERATION RELATION: DISK MASS AND THE DARK MATTER DISTRIBUTION
- Accepted to ApJ Preprint typeset using LATEX style emulateapj v. 03/07/07
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- A LIMIT ON THE COSMOLOGICAL MASS DENSITY AND POWER SPECTRUM FROM THE ROTATION CURVES OF LOW SURFACE BRIGHTNESS GALAXIES
- A POSSIBLE LOCAL COUNTERPART TO THE EXCESS POPULATION OF FAINT BLUE GALAXIES
- The Balance of Dark and Luminous Mass in Rotating Galaxies
- Dark Matter in the Universe, 1 October 2005 Stacy McGaugh
- DYNAMICAL STABILITY AND ENVIRONMENTAL INFLUENCES IN LOW SURFACE BRIGHTNESS DISK GALAXIES
- were attracted to ovules and entered the micropyle, but failed to burst and release
- The Connection Between Dark and Luminous Mass
- COULD A LOCAL GROUP X-RAY HALO AFFECT THE X-RAY AND MICROWAVE BACKGROUNDS? RACHEL A. PILDIS
- Empirical Constraints on Halo Profiles from Rotation Curves
- Mon. Not. R. Astron. Soc. 340, 657678 (2003) Simulating observations of dark matter dominated galaxies
- MILKY WAY MASS MODELS AND MOND Stacy S. McGaugh
- Ninety-five percent of the universe has gone missing.
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- A&A 490, 589600 (2008) DOI: 10.1051/0004-6361:200810410
- A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies Stacy S. McGaugh
- A&A 505, 577587 (2009) DOI: 10.1051/0004-6361/200811136
- MASS MODELS FOR LOW SURFACE BRIGHTNESS GALAXIES WITH HIGH-RESOLUTION OPTICAL VELOCITY FIELDS
- CONFRONTATION OF MODIFIED NEWTONIAN DYNAMICS PREDICTIONS WITH WILKINSON MICROWAVE ANISOTROPY PROBE FIRST YEAR DATA
- THE ROTATION VELOCITY ATTRIBUTABLE TO DARK MATTER AT INTERMEDIATE RADII IN DISK GALAXIES
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- The Rotation Velocity Attributable to Dark Matter at Intermediate Radii in Disk Galaxies
- Renzo's Rule: "For any feature in the luminosity profile there is a corresponding feature in the rotation curve and vice versa." (Sancisi 2004, IAU 220, 233)
- MOND: an Empiricist's Perspective Stacy McGaugh