Outputs (3)

Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters (2005)
Journal Article
Angulo, R., Baugh, C., Frenk, C., Bower, R., Jenkins, A., & Morris, S. (2005). Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters. Monthly Notices of the Royal Astronomical Society, 362(1), L25-L29. https://doi.org/10.1111/j.1745-3933.2005.00067.x

Acoustic oscillations in the baryon–photon fluid leave a signature in the matter power spectrum. The overall shape of the spectrum and the wavelength of the oscillations depend upon the sound horizon scale at recombination. Using the Λ cold dark matt... Read More about Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters.

The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3 (2005)
Journal Article
Wilman, R., Gerssen, J., Bower, R., Morris, S., Bacon, R., de Zeeuw, P., & Davies, R. (2005). The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3. Nature, 436(7048), 227-229. https://doi.org/10.1038/nature03718

High-velocity galactic outflows, driven by intense bursts of star formation and black hole accretion, are processes invoked by current theories of galaxy formation to terminate star formation in the most massive galaxies and to deposit heavy elements... Read More about The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z ≈ 3.

Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - I. Group properties. (2005)
Journal Article
Wilman, D., Balogh, M., Bower, R., Mulchaey, J., Oemler, A., Carlberg, R., …Whitaker, R. (2005). Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - I. Group properties. Monthly Notices of the Royal Astronomical Society, 358(1), 71-87. https://doi.org/10.1111/j.1365-2966.2005.08744.x

The evolution of galaxies in groups may have important implications for the evolution of the star formation history of the Universe, since many processes which operate in groups may suppress star formation and the fraction of galaxies in bound groups... Read More about Galaxy groups at 0.3 ⩽ z ⩽ 0.55 - I. Group properties..