1 |
Binney, J., & Tremaine, S. 2008, Galactic Dynamics, 2nd edn. (Princeton: Princeton University Press)
|
2 |
Bondi, H., & Samuel, J. 1997, The Lense-Thirring Effect and Mach's Principle, Phys. Letters A, 228, 121
DOI
ScienceOn
|
3 |
Cardone, V. F., Radicella, N., & Parisi, L. 2012, Constraining Massive Gravity with Recent Cosmological Data, Phys. Mod. Rev. D, 85, 124005
DOI
|
4 |
Dubinski, J., Mihos, J. C., & Hernquist, L. 1999, Constraining Dark Halo Potentials with Tidal Tails, ApJ, 526, 607
DOI
|
5 |
Bahcall, N. A., Ostriker, J. P., Perlmutter, S., & Steinhardt, P. J. 1999, The Cosmic Triangle: Revisiting the State of the Universe, Science, 284, 1481
DOI
ScienceOn
|
6 |
Barrena, R., Biviano, A., Ramella, M., Falco, E. E., & Seitz, S. 2002, The Dynamical Status of the Cluster of Galaxies 1E0657-56, A&A, 386, 816
DOI
ScienceOn
|
7 |
Faber, S. M., & Jackson, R. E. 1976, Velocity Dispersions and Mass-to-Light Ratios for Elliptical Galaxies, ApJ, 204, 668
DOI
|
8 |
Famaey, B., & McGaugh, S. S. 2012, Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions, Living Rev. Relativity, 15, 10
DOI
|
9 |
Gavazzi, R., Treu, T., Rhodes, J. D., et al. 2007, The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early-Type Galaxies out to 100 Effective Radii, ApJ, 667, 176
DOI
|
10 |
Goldhaber, A. S., & Nieto, M. M. 2010, Photon and Graviton Mass Limits, Rev. Mod. Phys., 82, 939
DOI
ScienceOn
|
11 |
Griffith, D. 2008, Introduction to Elementary Particles (Weinheim: Wiley-VCH)
|
12 |
Hernandez, X., & Lee, W. H. 2008, The Tightening of Wide Binaries in dSph Galaxies through Dynamical Friction as a Test of the Dark Matter Hypothesis, MNRAS, 387, 1727
DOI
ScienceOn
|
13 |
Hinterbichler, K. 2012, Theoretical Aspects of Massive Gravity, Rev. Mod. Phys., 84, 671
DOI
|
14 |
Jee, M. J., Mahdavi, A., Hoekstra, H., et al. 2012, A Study of the Dark Core in A520 with the Hubble Space Telescope: The Mystery Deepens, ApJ, 747, 96
DOI
|
15 |
Kim, J.-H., Park, C., Rossi, G., Lee, S. M., & Gott, J. R. III. 2011, The New Horizon Run Cosmological N-Body Simulations, JKAS, 44, 217
|
16 |
Kroupa, P. 2012, The Dark Matter Crisis: Falsification of the Current Standard Model of Cosmology, PASA, 29, 395
DOI
|
17 |
McGaugh, S. S. 2004, The Mass Discrepancy-Acceleration Relation: Disk Mass and the Dark Matter Distribution, ApJ, 609, 652
DOI
|
18 |
Lang, K. R. 2006, Astrophysical Formulae. Vol. I, 3rd edn. (Berlin: Springer)
|
19 |
Lee, J., & Komatsu, E. 2010, Bullet Cluster: a Challenge to ACDM Cosmology, ApJ, 718, 60
DOI
|
20 |
Markevitch, M., Govoni, F., Brunetti, G., & Jerius, D. 2005, Bow Shock and Radio Halo in the Merging Cluster A520, ApJ, 627, 733
DOI
|
21 |
Milgrom, M. 1983, A Modification of the Newtonian Dynamics as a Possible Alternative to the Hidden Mass Hypothesis, ApJ, 270, 365
DOI
|
22 |
Ostriker, J. P., & Peebles, P. J. E. 1973, A Numerical Study of the Stability of Flattened Galaxies: Or, Can Cold Galaxies Survive?, ApJ, 186, 467
DOI
|
23 |
Rubin, U. C., Ford, W. K. Jr., & Thonnard, N. 1980, Rotational Properties of 21 Sc Galaxies with a Large Range of Luminosities and Radii, from NGC4605 (R = 4 kpc) to UGC2885 (R = 122 kpc), ApJ, 238, 471
DOI
|
24 |
Sancisi, R. 2004, The Visible Matter - Dark Matter Coupling, in: Ryder, S. D., et al. (eds.), Dark Matter in Galaxies, IAU Symposium, 220, 233
|
25 |
Sparke, L. S., & Gallagher, J. S. III. 2007, Galaxies in the Universe, 2nd edn. (Cambridge: Cambridge University Press)
|
26 |
Tully, R. B., & Fisher, J. R. 1977, A New Method of Determining Distances to Galaxies, A&A, 54, 661
|
27 |
Zwicky, F. 1933, Die Rotverschiebung von Extragalaktischen Nebeln, Helvet. Phys. Acta, 6, 110
|