1 |
Bekenstein, J. & Milgrom, M., 1984, Does the Missing Mass Problem Signal the Breakdown of Newtonian Gravity?, ApJ, 286, 7
DOI
|
2 |
Blanton, M. R., Eisenstein, D., & Hogg, D. W., et al., 2005, Relationship between Environment and the Broadband Optical Properties of Galaxies in the Sloan Digital Sky Survey, ApJ, 629, 143
DOI
|
3 |
Cappellari, M., McDermid, R. M., & Alatalo, K., et al., 2012, Systematic variation of the stellar initial mass function in early-type galaxies, Nature, 484, 485
DOI
ScienceOn
|
4 |
Gallazzi, A., Charlot, S., & Brinchmann, J., et al., 2005, The Ages and Metallicities of Galaxies in the Local Universe, MNRAS, 362, 41
DOI
ScienceOn
|
5 |
Gallazzi, A. & Bell, E.F., 2009, Stellar Mass-to-Light Ratios from Galaxy Spectra: How Accurate can They be?, ApJS, 185, 253
DOI
|
6 |
Jiang, G. & Kochanek, C.S., 2007, The Baryon Fractions and Mass-to-Light Rations of Early-Tupe Galaxies, ApJ, 671, 1568
DOI
|
7 |
Kauffmann, G., Heckman, T. M., & White, S. D. M., et al., 2003a, Stellar Masses and Star Formation Histories for 105 Galaxies from the Sloan Digital Sky Survey, MNRAS, 341, 33
DOI
ScienceOn
|
8 |
Kauffmann, G., Heckman, T. M., & White, S. D. M., et al., 2003b, The Dependence of Star Formation History and Internal Structure on Stellar Mass for 105 Low-redshift Galaxies, MNRAS, 341, 54
DOI
ScienceOn
|
9 |
Milgrom, M., 1983, A Modication of the Newtonian Dynamics as a Possible Alternative to the Hidden Mass Hypothesis, ApJ, 270, 365
DOI
|
10 |
Shen, S., Mo, H.J., White, S.D.M., et al., 2003, The Size Distribution of Galaxies in the Sloan Digital Sky Survey, MNRAS, 343, 978
DOI
ScienceOn
|