Near-field cosmology

Science

Volumn 313, Issue 5785, 2006, Pages 311-312

  Bland Hawthorn, Joss ^a   Peebles, P J E ^b  

^a ANGLO AUSTRALIAN OBSERVATORY   (Australia)

^b PRINCETON UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COSMOLOGY;

ASTRONOMY; COMPUTER SIMULATION; COSMOS; PHYSICS; PRIORITY JOURNAL; REVIEW;

EID: 33749249574     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1127183     Document Type: Review

References (8)

1. Aspen Center for Physics workshop on Local Group Cosmology, Aspen, CO, 5 to 11 February 2006.
2. D. N. Spergel et al., http://arxiv.org/abs/astroph/0603449 (2006).
3. The Big Bang produced mostly hydrogen and helium, whereas most of the heavier elements were produced in stars and returned to the interstellar medium by supernovae and winds, in a process that cycled through generations of stars.
4. T. Beers, N. Christlieb, Annu. Rev. Astron. Astrophys. 43, 531 (2005).
5. A. R. Zentner, J. S. Bullock, Astrophys. J. 598, 49 (2003) and references therein.
6. B. Robertson et al., Astrophys. J. 632, 872 (2005).
7. German Astrophysical Virtual Observatory simulation query page (www.g-vo.org/mpasims).
8. V. Springel et al., Nature 435, 629 (2005).