Massive Galaxies and Central Black Holes at z = 6 to z = 8

Show more

References

[1] Steinhardt, C., et al. (2015) The Impossibly Early Galaxy Problem. arXiv:1506.01377.

[2] Planck Collaboration (2015) Planck 2015 Results. XIII. Cosmological Parameters. arXiv:1502.01589.

[3] Adler, R. and Overduin, J. (2005) General Relativity and Gravitation, 37, 1491. [gr-qc/0501061]

http://dx.doi.org/10.1007/s10714-005-0189-6

[4] Siemiginowska, A., et al. (2007) Astrophysical Journal, 657, 145.

http://dx.doi.org/10.1086/510898

[5] Bousso, R. (2002) Reviews of Modern Physics, 74, 825.

http://dx.doi.org/10.1103/RevModPhys.74.825

[6] Misner, C., Thorne, K. and Wheeler, J. (1973) Gravitation. W. H. Freeman and Company, New York.

[7] Mongan, T. (2012) Holography, Large Scale Structure, Supermassive Black Holes and Minimum Stellar Mass. arXiv:1301.0304.

[8] Longair, S. (1998) Galaxy Formation. Springer-Verlag, Berlin.

http://dx.doi.org/10.1007/978-3-662-03571-9

[9] Crowther, P. (2010) The R136 Star Cluster Hosts Several Stars Whose Individual Masses Greatly Exceed the Accepted 150 Msun Stellar Mass Limit. arXiv:1007.3284.

[10] Massey, P. and Meyer, R. (2001) Stellar Masses. Encyclopedia of Astronomy and Astrophysics.

http://dx.doi.org/10.1888/0333750888/1882

[11] Mortlock, D. (2011) Nature, 474, 616. [arXiv:1106.6088]

http://dx.doi.org/10.1038/nature10159

[12] Pacucci, F., Volonteri, M. and Ferrara, F. (2015) The Growth Efficiency of High-Redshift Black Holes. arXiv: 1506.04750.

http://dx.doi.org/10.1093/mnras/stv1465

[13] Trakhtenbrot, B., et al. (2015) Science, 349, 168. [arXiv:1507.02290]

http://dx.doi.org/10.1126/science.aaa4506