Feedback in low-mass galaxies in the early Universe
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/nature14454.pdf
Reference100 articles.
1. Burke, J. A. Mass flow from stellar systems—I. Radial flow from spherical systems. Mon. Not. R. Astron. Soc. 140, 241–254 (1968)
2. Pettini, M. et al. The rest-frame optical spectra of Lyman break galaxies: star formation, extinction, abundances, and kinematics. Astrophys. J. 554, 981–1000 (2001)This paper is the first study of rest-frame optical emission lines at z ≈ 3 that indicated the ubiquity and importance of galactic outflows.
3. Shapley, A. E., Steidel, C. C., Pettini, M. & Adelberger, K. L. Rest-frame ultraviolet spectra of z ≈ 3 Lyman break galaxies. Astrophys. J. 588, 65–89 (2003)This paper is a comprehensive study of the rest-frame ultraviolet spectra of star-forming galaxies at z ≈ 3, and demonstrates that the trends in the spectra arise from the properties of galactic outflows.
4. Weiner, B. J. et al. Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z = 1.4. Astrophys. J. 692, 187–211 (2009)
5. Steidel, C. C. et al. The structure and kinematics of the circumgalactic medium from far-ultraviolet spectra of z ≈ 2–3 galaxies. Astrophys. J. 717, 289–322 (2010)
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