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article · Astronomy and Astrophysics · 2007

Dust distribution during reionization

E. Elfgren, F.–X. Désert, B. Guiderdoni

Cited by 5Open access

Abstract

Context. The dust produced by the first generation of stars will be a foreground to cosmic microwave background.

Cite this paper

APA 7

Elfgren, E., Désert, F., & Guiderdoni, B. (2007). Dust distribution during reionization. Astronomy and Astrophysics, 476(3), 1145–1150. https://doi.org/10.1051/0004-6361:20053151

MLA 9

Elfgren, E., et al. “Dust distribution during reionization.” Astronomy and Astrophysics, vol. 476, no. 3, 2007, pp. 1145–50, https://doi.org/10.1051/0004-6361:20053151.

Chicago

Elfgren, E., F.–X. Désert, and B. Guiderdoni. 2007. “Dust distribution during reionization.” Astronomy and Astrophysics 476 (3): 1145–50. https://doi.org/10.1051/0004-6361:20053151.

Harvard

Elfgren, E., Désert, F. and Guiderdoni, B. (2007) ‘Dust distribution during reionization’, Astronomy and Astrophysics, 476(3), pp. 1145–1150. Available at: https://doi.org/10.1051/0004-6361:20053151.

BibTeX
@article{elfgren2007dust,
  title = {{Dust distribution during reionization}},
  author = {Elfgren, E. and Désert, F.–X. and Guiderdoni, B.},
  journal = {Astronomy and Astrophysics},
  volume = {476},
  number = {3},
  pages = {1145--1150},
  year = {2007},
  doi = {10.1051/0004-6361:20053151}
}

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